Morphological Characterization of Spiral Arms in Disk Galaxies from the IllustrisTNG50 Simulation and their Relation to the Properties of their Host Dark Matter Halos

We investigate the link between spiral structure and dark-matter halo properties in disk galaxies from the IllustrisTNG50 (ΛCDM) simulation. Disks were selected with kinematic filters; gas and stars were isolated, the mean density profile was computed, and the techniques of Barros Ramírez (2020) wer...

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Autores:
Certuche Grueso, Daniel Heraldo
Tipo de recurso:
Trabajo de grado de pregrado
Fecha de publicación:
2025
Institución:
Universidad de Antioquia
Repositorio:
Repositorio UdeA
Idioma:
eng
OAI Identifier:
oai:bibliotecadigital.udea.edu.co:10495/47724
Acceso en línea:
https://hdl.handle.net/10495/47724
Palabra clave:
Astronomía
Astronomy
Galaxias
Galaxies
Spiral Galaxies
Cosmological Simulations
Disk Dynamics
Morphological Characterization
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openAccess
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http://creativecommons.org/licenses/by-nc-sa/4.0/
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repository_id_str
dc.title.eng.fl_str_mv Morphological Characterization of Spiral Arms in Disk Galaxies from the IllustrisTNG50 Simulation and their Relation to the Properties of their Host Dark Matter Halos
title Morphological Characterization of Spiral Arms in Disk Galaxies from the IllustrisTNG50 Simulation and their Relation to the Properties of their Host Dark Matter Halos
spellingShingle Morphological Characterization of Spiral Arms in Disk Galaxies from the IllustrisTNG50 Simulation and their Relation to the Properties of their Host Dark Matter Halos
Astronomía
Astronomy
Galaxias
Galaxies
Spiral Galaxies
Cosmological Simulations
Disk Dynamics
Morphological Characterization
title_short Morphological Characterization of Spiral Arms in Disk Galaxies from the IllustrisTNG50 Simulation and their Relation to the Properties of their Host Dark Matter Halos
title_full Morphological Characterization of Spiral Arms in Disk Galaxies from the IllustrisTNG50 Simulation and their Relation to the Properties of their Host Dark Matter Halos
title_fullStr Morphological Characterization of Spiral Arms in Disk Galaxies from the IllustrisTNG50 Simulation and their Relation to the Properties of their Host Dark Matter Halos
title_full_unstemmed Morphological Characterization of Spiral Arms in Disk Galaxies from the IllustrisTNG50 Simulation and their Relation to the Properties of their Host Dark Matter Halos
title_sort Morphological Characterization of Spiral Arms in Disk Galaxies from the IllustrisTNG50 Simulation and their Relation to the Properties of their Host Dark Matter Halos
dc.creator.fl_str_mv Certuche Grueso, Daniel Heraldo
dc.contributor.advisor.none.fl_str_mv Muñoz Cuartas, Juan Carlos
dc.contributor.author.none.fl_str_mv Certuche Grueso, Daniel Heraldo
dc.contributor.researchgroup.none.fl_str_mv Grupo de Física y Astrofísica Computacional (FACOM)
dc.subject.lemb.none.fl_str_mv Astronomía
Astronomy
Galaxias
Galaxies
topic Astronomía
Astronomy
Galaxias
Galaxies
Spiral Galaxies
Cosmological Simulations
Disk Dynamics
Morphological Characterization
dc.subject.proposal.eng.fl_str_mv Spiral Galaxies
Cosmological Simulations
Disk Dynamics
Morphological Characterization
description We investigate the link between spiral structure and dark-matter halo properties in disk galaxies from the IllustrisTNG50 (ΛCDM) simulation. Disks were selected with kinematic filters; gas and stars were isolated, the mean density profile was computed, and the techniques of Barros Ramírez (2020) were adapted to characterize the spiral arms. An automated algorithm in polar coordinates, combining density-based clustering and graph theory, located arms defined as overdensities in the gas mass, and then quantified their width, length, and pitch angle. We show that these methods effectively identify spirals in isolated disks. We find that arm width increases with galactocentric radius, with a tracer-dependent gradient (gas is more sensitive). The pitch angle correlates positively with the galaxy’s mass components and negatively with subhalo concentration, suggesting that spiral geometry responds to the mass distribution and to the assembly history. Taken together, these results support the transient nature of spiral patterns and disk–halo coevolution, and represent a first step toward obtaining metrics that are comparable between simulations and observations. [Tomado de la introducción]
publishDate 2025
dc.date.accessioned.none.fl_str_mv 2025-10-14T15:51:17Z
dc.date.issued.none.fl_str_mv 2025
dc.date.available.none.fl_str_mv 2027
dc.type.none.fl_str_mv Trabajo de grado - Pregrado
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url https://hdl.handle.net/10495/47724
dc.language.iso.none.fl_str_mv eng
language eng
dc.relation.references.none.fl_str_mv M. G. Abadi et al. “Simulations of Galaxy Formation in a Λ Cold Dark Matter Universe. II. The Fine Structure of Simulated Galactic Disks”. In: The Astrophysical Journal 597.1 (2003), pp. 21–34. DOI: 10.1086/378316.
Brandon Allgood et al. “The shape of dark matter haloes: dependence on mass, redshift, radius and formation”. In: Monthly Notices of the Royal Astronomical Soci- ety 367.4 (2006), pp. 1781–1796.
David Felipe Barros-Ramirez and Juan Carlos Muñoz-Cuartas. “Star formation in disk galaxies and its relation with spiral structure in numerical simulations”. In: arXiv e-prints (2022), arXiv–2204.
Rainer Beck et al. “Galactic magnetism: recent developments and perspectives”. In: Annual review of astronomy and astrophysics 34.1 (1996), pp. 155–206.
Sidney Van den Bergh. Galaxy morphology and classification. Cambridge University Press, 1998.
James Binney and Scott Tremaine. Galactic dynamics. Princeton university press, 2011.
Bradley W Carroll and Dale A Ostlie. An introduction to modern astrophysics. Cam- bridge University Press, 2017.
JL Caswell and RF Haynes. “Southern H II regions. an extensive study of radio recombination line emission”. In: Astronomy and Astrophysics (ISSN 0004-6361), vol. 171, no. 1-2, Jan. 1987, p. 261-276. 171 (1987), pp. 261–276.
Thomas H. Cormen et al. Introduction to Algorithms. 2nd. The MIT Press, 2001. ISBN: 0262032937. URL: http://www.amazon.com/Introduction- Algorithms- Thomas-H-Cormen/dp/0262032937%3FSubscriptionId%3D13CT5CVB80YFWJEPWS02% 26tag%3Dws%26linkCode%3Dxm2%26camp%3D2025%26creative%3D165953%26creativeASIN%3D0262032937.
J. H. Croston et al. “XMM-Newton observations of the hot-gas atmospheres of 3C 66B and 3C 449”. In: Monthly Notices of the Royal Astronomical Society 346.4 (Dec. 2003), pp. 1041–1054. ISSN: 0035-8711. DOI: 10 . 1111 / j . 1365 - 2966 . 2003 . 07165 . x. eprint: https : / / academic . oup . com / mnras / article - pdf / 346 / 4 / 1041/18646083/346- 4- 1041.pdf. URL: https://doi.org/10.1111/j.1365- 2966.2003.07165.x.
DJ Croton et al. The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies. MNRAS. 2006.
Bruce G. Elmegreen. “What triggers star formation in galaxies?” In: Proceedings of the International Astronomical Union 7.S284 (2011), 317–329. DOI: 10.1017/S1743921312009350
Debra Meloy Elmegreen and Bruce G Elmegreen. “Flocculent and grand design spiral structure in field, binary and group galaxies”. In: Monthly Notices of the Royal Astronomical Society 201.4 (1982), pp. 1021–1034.
Martin Ester et al. “A density-based algorithm for discovering clusters in large spatial databases with noise”. In: kdd. Vol. 96. 34. 1996, pp. 226–231.
Ignacio Ferreras. Fundamentals of Galaxy Dynamics, Formation and Evolution. UCL Press, 2019.
Kenneth C Freeman. “On the disks of spiral and S0 galaxies”. In: Astrophysical Journal, vol. 160, p. 811 160 (1970), p. 811.
Yo M Georgelin and YP Georgelin. “The spiral structure of our Galaxy determined from H II regions”. In: Astronomy and Astrophysics, vol. 49, no. 1, May 1976, p. 57-79. Translation. 49 (1976), pp. 57–79.
Fabio Governato et al. “Bulgeless dwarf galaxies and dark matter cores from supernova- driven outflows”. In: nature 463.7278 (2010), pp. 203–206.
Ross E. Hart et al. “Galaxy Zoo: comparing the demographics of spiral arm number and a new method for correcting redshift bias”. In: Monthly Notices of the Royal Astronomical Society 461.4 (July 2016), pp. 3663–3682. ISSN: 0035-8711. DOI: 10.1093/mnras/stw1588. eprint: https://academic.oup.com/mnras/article- pdf/461/4/3663/8112546/stw1588.pdf. URL: https://doi.org/10.1093/mnras/ stw1588.
Ross E Hart et al. “Galaxy Zoo: star formation versus spiral arm number”. In: Monthly Notices of the Royal Astronomical Society 468.2 (2017), pp. 1850–1863.
Lars Hernquist. “An analytical model for spherical galaxies and bulges”. In: Astro- physical Journal, Part 1 (ISSN 0004-637X), vol. 356, June 20, 1990, p. 359-364. 356 (1990), pp. 359–364.
Frank Hohl. “Numerical experiments with a disk of stars”. In: Astrophysical Journal, vol. 168, p. 343 168 (1971), p. 343.
Z. N. Honig and M. J. Reid. “Characteristics of Spiral Arms in Late-type Galaxies”. In: 800.1, 53 (Feb. 2015), p. 53. DOI: 10 . 1088 / 0004 - 637X / 800 / 1 / 53. arXiv: 1412.1012 [astro-ph.GA].
Michael Hoskin. “The first drawing of a spiral nebula”. In: Journal for the History of Astronomy 13.2 (1982), pp. 97–101.
LG Hou and JL Han. “The observed spiral structure of the Milky Way”. In: Astron- omy & Astrophysics 569 (2014), A125
E. P. Hubble. “Extragalactic nebulae”. In: The Astrophysical Journal 64 (1926).
llustrisTNG Collaboration. IllustrisTNG Project Description. https : / / www . tng - project.org/about/. Accessed: 2025-09-01. 2025.
Fabio Andrés Cardona Jaramillo. “About galactic disk formation and the relation between satellite orbital parameters and the morphology of the host galaxy”. Fac- ulty of Exact and Natural Sciences, Institute of Physics. Master’s thesis. Medellín, Colombia: University of Antioquia, 2021.
TH Jarrett et al. “The 2MASS large galaxy atlas”. In: The Astronomical Journal 125.2 (2003), p. 525.
Michele Kaufman et al. “A comparison of spiral tracers in M81”. In: Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 345, Oct. 15, 1989, p. 674-696. 345 (1989), pp. 674–696.
Russell M Kulsrud. Plasma physics for astrophysics. Princeton University Press, 2005.
Chin Yang Lee. “An algorithm for path connections and its applications”. In: IRE transactions on electronic computers 3 (2009), pp. 346–365.
Charles E Leiserson and Tao B Schardl. “A work-efficient parallel breadth-first search algorithm (or how to cope with the nondeterminism of reducers)”. In: Pro- ceedings of the twenty-second annual ACM symposium on Parallelism in algorithms and architectures. 2010, pp. 303–314.
CC Lin and FH-S Shu. “Density wave theory of spiral structure”. In: Selected Papers of CC Lin with Commentary: Vol. 1: Fluid Mechanics Vol. 2: Astrophysics. World Scientific, 1987, pp. 645–743.
Donald Lynden-Bell and Jim E Pringle. “The evolution of viscous discs and the ori- gin of the nebular variables”. In: Monthly Notices of the Royal Astronomical Society 168.3 (1974), pp. 603–637,
Andrea V Maccio et al. “Abundance matching tested on small scales with galaxy dynamics”. In: Monthly Notices of the Royal Astronomical Society: Letters 496.1 (2020), pp. L101–L105.
Andrea V. Macciò et al. “Concentration, spin and shape of dark matter haloes: scatter and the dependence on mass and environment”. In: Monthly Notices of the Royal Astronomical Society 378.1 (May 2007), pp. 55–71. ISSN: 0035-8711. DOI: 10. 1111/j. 1365- 2966.2007 .11720.x. eprint: https: //academic. oup.com / mnras / article - pdf / 378 / 1 / 55 / 3960691 / mnras0378 - 0055 . pdf. URL: https : //doi.org/10.1111/j.1365-2966.2007.11720.x.
Ariyeh H Maller and Avishai Dekel. “Towards a resolution of the galactic spin cri- sis: mergers, feedback and spin segregation”. In: Monthly Notices of the Royal As- tronomical Society 335.2 (2002), pp. 487–498.
H. J. Mo, Shude Mao, and Simon D. M. White. “The formation of galactic discs”. In: Monthly Notices of the Royal Astronomical Society 295.2 (Apr. 1998), pp. 319– 336. ISSN: 0035-8711. DOI: 10.1046/j.1365-8711.1998.01227.x. eprint: https: //academic.oup.com/mnras/article-pdf/295/2/319/3099899/295-2-319.pdf. URL: https://doi.org/10.1046/j.1365-8711.1998.01227.x.
HJ Mo, Shude Mao, and Simon DM White. “The formation of galactic discs”. In: Monthly Notices of the Royal Astronomical Society 295.2 (1998), pp. 319–336.
Edward F Moore. “The shortest path through a maze”. In: Proc. of the International Symposium on the Theory of Switching. Harvard University Press. 1959, pp. 285– 292.
J. C. Muñoz-Cuartas et al. “The redshift evolution of cold dark matter halo param- eters: concentration, spin and shape”. In: Monthly Notices of the Royal Astronomical Society 411.1 (Jan. 2011), pp. 584–594. ISSN: 0035-8711. DOI: 10.1111/j.1365- 2966 . 2010 . 17704 . x. eprint: https : / / academic . oup . com / mnras / article - pdf/411/1/584/3534439/mnras0411- 0584.pdf. URL: https://doi.org/10. 1111/j.1365-2966.2010.17704.x.
Julio F. Navarro, Carlos S. Frenk, and Simon D. M. White. “Simulations of X-ray clusters”. In: Monthly Notices of the Royal Astronomical Society 275.3 (Aug. 1995), pp. 720–740. ISSN: 0035-8711. DOI: 10.1093/mnras/275.3.720. eprint: https: / / academic . oup . com / mnras / article - pdf / 275 / 3 / 720 / 2805863 / mnras275 - 0720.pdf. URL: https://doi.org/10.1093/mnras/275.3.720.
D. Nelson et al. “First results from the IllustrisTNG simulations: the galaxy colour bimodality”. In: Monthly Notices of the Royal Astronomical Society 475.1 (Nov. 2017), pp. 624–647. DOI: 10 . 1093 / mnras / stx3040. arXiv: arXiv : 1707 . 03395 [astro-ph.CO]. URL: https://doi.org/10.1093/mnras/stx3040.
Dylan Nelson et al. “First results from the TNG50 simulation: galactic outflows driven by supernovae and black hole feedback”. In: 490.3 (Dec. 2019), pp. 3234– 3261. DOI: 10.1093/mnras/stz2306. arXiv: 1902.05554 [astro-ph.GA].
Annalisa Pillepich et al. “First results from the TNG50 simulation: the evolution of stellar and gaseous discs across cosmic time”. In: Monthly Notices of the Royal Astronomical Society 490.3 (2019), pp. 3196–3233.
Annalisa Pillepich et al. “First results from the TNG50 simulation: the evolution of stellar and gaseous discs across cosmic time”. In: 490.3 (Dec. 2019), pp. 3196– 3233. DOI: 10.1093/mnras/stz2338. arXiv: 1902.05553 [astro-ph.GA].
Annalisa Pillepich et al. “Simulating galaxy formation with the IllustrisTNG model”. In: 473.3 (Jan. 2018), pp. 4077–4106. DOI: 10 . 1093 / mnras / stx2656. arXiv: 1703.02970 [astro-ph.GA].
Planck Collaboration et al. “Planck 2015 results. XIII. Cosmological parameters”. In: 594, A13 (Sept. 2016), A13. DOI: 10 . 1051 / 0004 - 6361 / 201525830. arXiv: 1502.01589 [astro-ph.CO].
Lorenzo Posti et al. “Galaxy disc scaling relations: A tight linear galaxy–halo con- nection challenges abundance matching”. In: Astronomy & Astrophysics 629 (2019), A59.
Lorenzo Posti et al. “Galaxy spin as a formation probe: the stellar-to-halo specific angular momentum relation”. In: 475.1 (Mar. 2018), pp. 232–243. DOI: 10.1093/ mnras/stx3168. arXiv: 1711.04763 [astro-ph.GA].
Harry I. Ringermacher and Lawrence R. Mead. “A new formula describing the scaffold structure of spiral galaxies”. In: Monthly Notices of the Royal Astronomical Society 397.1 (July 2009), pp. 164–171. ISSN: 0035-8711. DOI: 10.1111/j.1365- 2966 . 2009 . 14950 . x. eprint: https : / / academic . oup . com / mnras / article - pdf/397/1/164/18431940/mnras0397- 0164.pdf. URL: https://doi.org/10. 1111/j.1365-2966.2009.14950.x.
D Russeil. “Star-forming complexes and the spiral structure of our Galaxy”. In: Astronomy & Astrophysics 397.1 (2003), pp. 133–146.
Allan Sandage. The Hubble atlas of galaxies. Vol. 618. 2. Carnegie Institution of Washington Washington, DC, 1961.
Eva Schinnerer et al. “The PdBI Arcsecond Whirlpool Survey (PAWS). I. A cloud- scale/multi-wavelength view of the interstellar medium in a grand-design spiral galaxy”. In: The Astrophysical Journal 779.1 (2013), p. 42.
Peter Schneider. Extragalactic astronomy and cosmology: an introduction. Vol. 146. Springer, 2006.
Jerry A Sellwood and Karen L Masters. “Spirals in galaxies”. In: Annual Review of Astronomy and Astrophysics 60.1 (2022), pp. 73–120.
E. Silva-Villa and X. Cano Gómez. “NGC 5236’s stars as tracers of arms and arm widths in spiral galaxies”. In: Monthly Notices of the Royal Astronomical Society: Letters 514.1 (2022), pp. L22–L26.
E. Silva-Villa and S. S. Larsen. “A study of the cluster formation history in M83 using the luminosity function and mass function”. In: Astronomy & Astrophysics 537 (2012), A145.
Yoshiaki Sofue and Vera Rubin. “Rotation curves of spiral galaxies”. In: Annual Review of Astronomy and Astrophysics 39.1 (2001), pp. 137–174.
Rachel S Somerville and Romeel Davé. “Physical models of galaxy formation in a cosmological framework”. In: Annual Review of Astronomy and Astrophysics 53.1 (2015), pp. 51–113.
Jesper Sommer-Larsen, Sergio Gelato, and Henrik Vedel. “Formation of disk galax- ies: feedback and the angular momentum problem”. In: The Astrophysical Journal 519.2 (1999), p. 501.
Volker Springel. “Moving-mesh hydrodynamics with the AREPO code”. In: Proceed- ings of the International Astronomical Union 6.S270 (2010), pp. 203–206.
Iskra Strateva et al. “Color separation of galaxy types in the Sloan Digital Sky Survey imaging data”. In: The Astronomical Journal 122.4 (2001), p. 1861.
Alar Toomre. “On the gravitational stability of a disk of stars”. In: Astrophysical Journal, vol. 139, p. 1217-1238 (1964). 139 (1964), pp. 1217–1238.
R Brent Tully and J Richard Fisher. “A new method of determining distances to galaxies”. In: Astronomy and Astrophysics, vol. 54, no. 3, Feb. 1977, p. 661-673. 54 (1977), pp. 661–673.
Frank C Van Den Bosch, Andreas Burkert, and Rob A Swaters. “The angular mo- mentum content of dwarf galaxies: new challenges for the theory of galaxy forma- tion”. In: Monthly Notices of the Royal Astronomical Society 326.3 (2001), pp. 1205– 1215.
Mark Vogelsberger et al. “Introducing the Illustris Project: simulating the coevolu- tion of dark and visible matter in the Universe”. In: Monthly Notices of the Royal Astronomical Society 444.2 (2014), pp. 1518–1547.
Risa H Wechsler and Jeremy L Tinker. “The connection between galaxies and their dark matter halos”. In: Annual Review of Astronomy and Astrophysics 56.1 (2018), pp. 435–487.
Rainer Weinberger et al. “Simulating galaxy formation with black hole driven ther- mal and kinetic feedback”. In: 465.3 (Mar. 2017), pp. 3291–3308. DOI: 10.1093/ mnras/stw2944. arXiv: 1607.03486 [astro-ph.GA].
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spelling Muñoz Cuartas, Juan CarlosCertuche Grueso, Daniel HeraldoGrupo de Física y Astrofísica Computacional (FACOM)2025-10-14T15:51:17Z20272025https://hdl.handle.net/10495/47724We investigate the link between spiral structure and dark-matter halo properties in disk galaxies from the IllustrisTNG50 (ΛCDM) simulation. Disks were selected with kinematic filters; gas and stars were isolated, the mean density profile was computed, and the techniques of Barros Ramírez (2020) were adapted to characterize the spiral arms. An automated algorithm in polar coordinates, combining density-based clustering and graph theory, located arms defined as overdensities in the gas mass, and then quantified their width, length, and pitch angle. We show that these methods effectively identify spirals in isolated disks. We find that arm width increases with galactocentric radius, with a tracer-dependent gradient (gas is more sensitive). The pitch angle correlates positively with the galaxy’s mass components and negatively with subhalo concentration, suggesting that spiral geometry responds to the mass distribution and to the assembly history. Taken together, these results support the transient nature of spiral patterns and disk–halo coevolution, and represent a first step toward obtaining metrics that are comparable between simulations and observations. [Tomado de la introducción]COL0038262PregradoAstrónomo77 páginasapplication/pdfengUniversidad de AntioquiaAstronomíaDepartamento de Ciencias BásicasMedellín, ColombiaFacultad de Ciencias Exactas y NaturalesCampus Medellín - Ciudad Universitariahttp://creativecommons.org/licenses/by-nc-sa/4.0/info:eu-repo/semantics/openAccessAttribution-NonCommercial-ShareAlike 4.0 Internationalhttp://purl.org/coar/access_right/c_abf2Morphological Characterization of Spiral Arms in Disk Galaxies from the IllustrisTNG50 Simulation and their Relation to the Properties of their Host Dark Matter HalosTrabajo de grado - Pregradohttp://purl.org/coar/resource_type/c_7a1fhttp://purl.org/redcol/resource_type/TPTexthttp://purl.org/coar/version/c_b1a7d7d4d402bcceinfo:eu-repo/semantics/bachelorThesisinfo:eu-repo/semantics/draftM. G. Abadi et al. “Simulations of Galaxy Formation in a Λ Cold Dark Matter Universe. II. The Fine Structure of Simulated Galactic Disks”. In: The Astrophysical Journal 597.1 (2003), pp. 21–34. DOI: 10.1086/378316.Brandon Allgood et al. “The shape of dark matter haloes: dependence on mass, redshift, radius and formation”. In: Monthly Notices of the Royal Astronomical Soci- ety 367.4 (2006), pp. 1781–1796.David Felipe Barros-Ramirez and Juan Carlos Muñoz-Cuartas. “Star formation in disk galaxies and its relation with spiral structure in numerical simulations”. In: arXiv e-prints (2022), arXiv–2204.Rainer Beck et al. “Galactic magnetism: recent developments and perspectives”. In: Annual review of astronomy and astrophysics 34.1 (1996), pp. 155–206.Sidney Van den Bergh. Galaxy morphology and classification. Cambridge University Press, 1998.James Binney and Scott Tremaine. Galactic dynamics. Princeton university press, 2011.Bradley W Carroll and Dale A Ostlie. An introduction to modern astrophysics. Cam- bridge University Press, 2017.JL Caswell and RF Haynes. “Southern H II regions. an extensive study of radio recombination line emission”. In: Astronomy and Astrophysics (ISSN 0004-6361), vol. 171, no. 1-2, Jan. 1987, p. 261-276. 171 (1987), pp. 261–276.Thomas H. Cormen et al. Introduction to Algorithms. 2nd. The MIT Press, 2001. ISBN: 0262032937. URL: http://www.amazon.com/Introduction- Algorithms- Thomas-H-Cormen/dp/0262032937%3FSubscriptionId%3D13CT5CVB80YFWJEPWS02% 26tag%3Dws%26linkCode%3Dxm2%26camp%3D2025%26creative%3D165953%26creativeASIN%3D0262032937.J. H. Croston et al. “XMM-Newton observations of the hot-gas atmospheres of 3C 66B and 3C 449”. In: Monthly Notices of the Royal Astronomical Society 346.4 (Dec. 2003), pp. 1041–1054. ISSN: 0035-8711. DOI: 10 . 1111 / j . 1365 - 2966 . 2003 . 07165 . x. eprint: https : / / academic . oup . com / mnras / article - pdf / 346 / 4 / 1041/18646083/346- 4- 1041.pdf. URL: https://doi.org/10.1111/j.1365- 2966.2003.07165.x.DJ Croton et al. The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies. MNRAS. 2006.Bruce G. Elmegreen. “What triggers star formation in galaxies?” In: Proceedings of the International Astronomical Union 7.S284 (2011), 317–329. DOI: 10.1017/S1743921312009350Debra Meloy Elmegreen and Bruce G Elmegreen. “Flocculent and grand design spiral structure in field, binary and group galaxies”. In: Monthly Notices of the Royal Astronomical Society 201.4 (1982), pp. 1021–1034.Martin Ester et al. “A density-based algorithm for discovering clusters in large spatial databases with noise”. In: kdd. Vol. 96. 34. 1996, pp. 226–231.Ignacio Ferreras. Fundamentals of Galaxy Dynamics, Formation and Evolution. UCL Press, 2019.Kenneth C Freeman. “On the disks of spiral and S0 galaxies”. In: Astrophysical Journal, vol. 160, p. 811 160 (1970), p. 811.Yo M Georgelin and YP Georgelin. “The spiral structure of our Galaxy determined from H II regions”. In: Astronomy and Astrophysics, vol. 49, no. 1, May 1976, p. 57-79. Translation. 49 (1976), pp. 57–79.Fabio Governato et al. “Bulgeless dwarf galaxies and dark matter cores from supernova- driven outflows”. In: nature 463.7278 (2010), pp. 203–206.Ross E. Hart et al. “Galaxy Zoo: comparing the demographics of spiral arm number and a new method for correcting redshift bias”. In: Monthly Notices of the Royal Astronomical Society 461.4 (July 2016), pp. 3663–3682. ISSN: 0035-8711. DOI: 10.1093/mnras/stw1588. eprint: https://academic.oup.com/mnras/article- pdf/461/4/3663/8112546/stw1588.pdf. URL: https://doi.org/10.1093/mnras/ stw1588.Ross E Hart et al. “Galaxy Zoo: star formation versus spiral arm number”. In: Monthly Notices of the Royal Astronomical Society 468.2 (2017), pp. 1850–1863.Lars Hernquist. “An analytical model for spherical galaxies and bulges”. In: Astro- physical Journal, Part 1 (ISSN 0004-637X), vol. 356, June 20, 1990, p. 359-364. 356 (1990), pp. 359–364.Frank Hohl. “Numerical experiments with a disk of stars”. In: Astrophysical Journal, vol. 168, p. 343 168 (1971), p. 343.Z. N. Honig and M. J. Reid. “Characteristics of Spiral Arms in Late-type Galaxies”. In: 800.1, 53 (Feb. 2015), p. 53. DOI: 10 . 1088 / 0004 - 637X / 800 / 1 / 53. arXiv: 1412.1012 [astro-ph.GA].Michael Hoskin. “The first drawing of a spiral nebula”. In: Journal for the History of Astronomy 13.2 (1982), pp. 97–101.LG Hou and JL Han. “The observed spiral structure of the Milky Way”. In: Astron- omy & Astrophysics 569 (2014), A125E. P. Hubble. “Extragalactic nebulae”. In: The Astrophysical Journal 64 (1926).llustrisTNG Collaboration. IllustrisTNG Project Description. https : / / www . tng - project.org/about/. Accessed: 2025-09-01. 2025.Fabio Andrés Cardona Jaramillo. “About galactic disk formation and the relation between satellite orbital parameters and the morphology of the host galaxy”. Fac- ulty of Exact and Natural Sciences, Institute of Physics. Master’s thesis. Medellín, Colombia: University of Antioquia, 2021.TH Jarrett et al. “The 2MASS large galaxy atlas”. In: The Astronomical Journal 125.2 (2003), p. 525.Michele Kaufman et al. “A comparison of spiral tracers in M81”. In: Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 345, Oct. 15, 1989, p. 674-696. 345 (1989), pp. 674–696.Russell M Kulsrud. Plasma physics for astrophysics. Princeton University Press, 2005.Chin Yang Lee. “An algorithm for path connections and its applications”. In: IRE transactions on electronic computers 3 (2009), pp. 346–365.Charles E Leiserson and Tao B Schardl. “A work-efficient parallel breadth-first search algorithm (or how to cope with the nondeterminism of reducers)”. In: Pro- ceedings of the twenty-second annual ACM symposium on Parallelism in algorithms and architectures. 2010, pp. 303–314.CC Lin and FH-S Shu. “Density wave theory of spiral structure”. In: Selected Papers of CC Lin with Commentary: Vol. 1: Fluid Mechanics Vol. 2: Astrophysics. World Scientific, 1987, pp. 645–743.Donald Lynden-Bell and Jim E Pringle. “The evolution of viscous discs and the ori- gin of the nebular variables”. In: Monthly Notices of the Royal Astronomical Society 168.3 (1974), pp. 603–637,Andrea V Maccio et al. “Abundance matching tested on small scales with galaxy dynamics”. In: Monthly Notices of the Royal Astronomical Society: Letters 496.1 (2020), pp. L101–L105.Andrea V. Macciò et al. “Concentration, spin and shape of dark matter haloes: scatter and the dependence on mass and environment”. In: Monthly Notices of the Royal Astronomical Society 378.1 (May 2007), pp. 55–71. ISSN: 0035-8711. DOI: 10. 1111/j. 1365- 2966.2007 .11720.x. eprint: https: //academic. oup.com / mnras / article - pdf / 378 / 1 / 55 / 3960691 / mnras0378 - 0055 . pdf. URL: https : //doi.org/10.1111/j.1365-2966.2007.11720.x.Ariyeh H Maller and Avishai Dekel. “Towards a resolution of the galactic spin cri- sis: mergers, feedback and spin segregation”. In: Monthly Notices of the Royal As- tronomical Society 335.2 (2002), pp. 487–498.H. J. Mo, Shude Mao, and Simon D. M. White. “The formation of galactic discs”. In: Monthly Notices of the Royal Astronomical Society 295.2 (Apr. 1998), pp. 319– 336. ISSN: 0035-8711. DOI: 10.1046/j.1365-8711.1998.01227.x. eprint: https: //academic.oup.com/mnras/article-pdf/295/2/319/3099899/295-2-319.pdf. URL: https://doi.org/10.1046/j.1365-8711.1998.01227.x.HJ Mo, Shude Mao, and Simon DM White. “The formation of galactic discs”. In: Monthly Notices of the Royal Astronomical Society 295.2 (1998), pp. 319–336.Edward F Moore. “The shortest path through a maze”. In: Proc. of the International Symposium on the Theory of Switching. Harvard University Press. 1959, pp. 285– 292.J. C. Muñoz-Cuartas et al. “The redshift evolution of cold dark matter halo param- eters: concentration, spin and shape”. In: Monthly Notices of the Royal Astronomical Society 411.1 (Jan. 2011), pp. 584–594. ISSN: 0035-8711. DOI: 10.1111/j.1365- 2966 . 2010 . 17704 . x. eprint: https : / / academic . oup . com / mnras / article - pdf/411/1/584/3534439/mnras0411- 0584.pdf. URL: https://doi.org/10. 1111/j.1365-2966.2010.17704.x.Julio F. Navarro, Carlos S. Frenk, and Simon D. M. White. “Simulations of X-ray clusters”. In: Monthly Notices of the Royal Astronomical Society 275.3 (Aug. 1995), pp. 720–740. ISSN: 0035-8711. DOI: 10.1093/mnras/275.3.720. eprint: https: / / academic . oup . com / mnras / article - pdf / 275 / 3 / 720 / 2805863 / mnras275 - 0720.pdf. URL: https://doi.org/10.1093/mnras/275.3.720.D. Nelson et al. “First results from the IllustrisTNG simulations: the galaxy colour bimodality”. In: Monthly Notices of the Royal Astronomical Society 475.1 (Nov. 2017), pp. 624–647. DOI: 10 . 1093 / mnras / stx3040. arXiv: arXiv : 1707 . 03395 [astro-ph.CO]. URL: https://doi.org/10.1093/mnras/stx3040.Dylan Nelson et al. “First results from the TNG50 simulation: galactic outflows driven by supernovae and black hole feedback”. In: 490.3 (Dec. 2019), pp. 3234– 3261. DOI: 10.1093/mnras/stz2306. arXiv: 1902.05554 [astro-ph.GA].Annalisa Pillepich et al. “First results from the TNG50 simulation: the evolution of stellar and gaseous discs across cosmic time”. In: Monthly Notices of the Royal Astronomical Society 490.3 (2019), pp. 3196–3233.Annalisa Pillepich et al. “First results from the TNG50 simulation: the evolution of stellar and gaseous discs across cosmic time”. In: 490.3 (Dec. 2019), pp. 3196– 3233. DOI: 10.1093/mnras/stz2338. arXiv: 1902.05553 [astro-ph.GA].Annalisa Pillepich et al. “Simulating galaxy formation with the IllustrisTNG model”. In: 473.3 (Jan. 2018), pp. 4077–4106. DOI: 10 . 1093 / mnras / stx2656. arXiv: 1703.02970 [astro-ph.GA].Planck Collaboration et al. “Planck 2015 results. XIII. Cosmological parameters”. In: 594, A13 (Sept. 2016), A13. DOI: 10 . 1051 / 0004 - 6361 / 201525830. arXiv: 1502.01589 [astro-ph.CO].Lorenzo Posti et al. “Galaxy disc scaling relations: A tight linear galaxy–halo con- nection challenges abundance matching”. In: Astronomy & Astrophysics 629 (2019), A59.Lorenzo Posti et al. “Galaxy spin as a formation probe: the stellar-to-halo specific angular momentum relation”. In: 475.1 (Mar. 2018), pp. 232–243. DOI: 10.1093/ mnras/stx3168. arXiv: 1711.04763 [astro-ph.GA].Harry I. Ringermacher and Lawrence R. Mead. “A new formula describing the scaffold structure of spiral galaxies”. In: Monthly Notices of the Royal Astronomical Society 397.1 (July 2009), pp. 164–171. ISSN: 0035-8711. DOI: 10.1111/j.1365- 2966 . 2009 . 14950 . x. eprint: https : / / academic . oup . com / mnras / article - pdf/397/1/164/18431940/mnras0397- 0164.pdf. URL: https://doi.org/10. 1111/j.1365-2966.2009.14950.x.D Russeil. “Star-forming complexes and the spiral structure of our Galaxy”. In: Astronomy & Astrophysics 397.1 (2003), pp. 133–146.Allan Sandage. The Hubble atlas of galaxies. Vol. 618. 2. Carnegie Institution of Washington Washington, DC, 1961.Eva Schinnerer et al. “The PdBI Arcsecond Whirlpool Survey (PAWS). I. A cloud- scale/multi-wavelength view of the interstellar medium in a grand-design spiral galaxy”. In: The Astrophysical Journal 779.1 (2013), p. 42.Peter Schneider. Extragalactic astronomy and cosmology: an introduction. Vol. 146. Springer, 2006.Jerry A Sellwood and Karen L Masters. “Spirals in galaxies”. In: Annual Review of Astronomy and Astrophysics 60.1 (2022), pp. 73–120.E. Silva-Villa and X. Cano Gómez. “NGC 5236’s stars as tracers of arms and arm widths in spiral galaxies”. In: Monthly Notices of the Royal Astronomical Society: Letters 514.1 (2022), pp. L22–L26.E. Silva-Villa and S. S. Larsen. “A study of the cluster formation history in M83 using the luminosity function and mass function”. In: Astronomy & Astrophysics 537 (2012), A145.Yoshiaki Sofue and Vera Rubin. “Rotation curves of spiral galaxies”. In: Annual Review of Astronomy and Astrophysics 39.1 (2001), pp. 137–174.Rachel S Somerville and Romeel Davé. “Physical models of galaxy formation in a cosmological framework”. In: Annual Review of Astronomy and Astrophysics 53.1 (2015), pp. 51–113.Jesper Sommer-Larsen, Sergio Gelato, and Henrik Vedel. “Formation of disk galax- ies: feedback and the angular momentum problem”. In: The Astrophysical Journal 519.2 (1999), p. 501.Volker Springel. “Moving-mesh hydrodynamics with the AREPO code”. In: Proceed- ings of the International Astronomical Union 6.S270 (2010), pp. 203–206.Iskra Strateva et al. “Color separation of galaxy types in the Sloan Digital Sky Survey imaging data”. In: The Astronomical Journal 122.4 (2001), p. 1861.Alar Toomre. “On the gravitational stability of a disk of stars”. In: Astrophysical Journal, vol. 139, p. 1217-1238 (1964). 139 (1964), pp. 1217–1238.R Brent Tully and J Richard Fisher. “A new method of determining distances to galaxies”. In: Astronomy and Astrophysics, vol. 54, no. 3, Feb. 1977, p. 661-673. 54 (1977), pp. 661–673.Frank C Van Den Bosch, Andreas Burkert, and Rob A Swaters. “The angular mo- mentum content of dwarf galaxies: new challenges for the theory of galaxy forma- tion”. In: Monthly Notices of the Royal Astronomical Society 326.3 (2001), pp. 1205– 1215.Mark Vogelsberger et al. “Introducing the Illustris Project: simulating the coevolu- tion of dark and visible matter in the Universe”. In: Monthly Notices of the Royal Astronomical Society 444.2 (2014), pp. 1518–1547.Risa H Wechsler and Jeremy L Tinker. “The connection between galaxies and their dark matter halos”. In: Annual Review of Astronomy and Astrophysics 56.1 (2018), pp. 435–487.Rainer Weinberger et al. “Simulating galaxy formation with black hole driven ther- mal and kinetic feedback”. In: 465.3 (Mar. 2017), pp. 3291–3308. 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