Structural analysis of massive protoclusters formed from cloud collision

Este proyecto inició como parte de Chalmers Astrophysics & Space Science Summer (CASSUM) Research Fellowship

Autores:: García Alvarado, María Valentina

Tipo de recurso:: Trabajo de grado de pregrado

Fecha de publicación:: 2022

Institución:: Universidad de los Andes

Repositorio:: Séneca: repositorio Uniandes

Idioma:: eng

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dc.title.none.fl_str_mv	Structural analysis of massive protoclusters formed from cloud collision
title	Structural analysis of massive protoclusters formed from cloud collision
spellingShingle	Structural analysis of massive protoclusters formed from cloud collision Formación estelar Nubes moleculares gigantes Campo magnético Simulaciones Colisión Física
title_short	Structural analysis of massive protoclusters formed from cloud collision
title_full	Structural analysis of massive protoclusters formed from cloud collision
title_fullStr	Structural analysis of massive protoclusters formed from cloud collision
title_full_unstemmed	Structural analysis of massive protoclusters formed from cloud collision
title_sort	Structural analysis of massive protoclusters formed from cloud collision
dc.creator.fl_str_mv	García Alvarado, María Valentina
dc.contributor.advisor.none.fl_str_mv	Tan, Jonathan Forero Romero, Jaime Ernesto
dc.contributor.author.none.fl_str_mv	García Alvarado, María Valentina
dc.contributor.jury.none.fl_str_mv	García Varela, José Alejandro
dc.subject.keyword.none.fl_str_mv	Formación estelar Nubes moleculares gigantes Campo magnético Simulaciones Colisión
topic	Formación estelar Nubes moleculares gigantes Campo magnético Simulaciones Colisión Física
dc.subject.themes.es_CO.fl_str_mv	Física
description	Este proyecto inició como parte de Chalmers Astrophysics & Space Science Summer (CASSUM) Research Fellowship
publishDate	2022
dc.date.issued.none.fl_str_mv	2022-12-15
dc.date.accessioned.none.fl_str_mv	2023-01-27T16:27:50Z
dc.date.available.none.fl_str_mv	2023-01-27T16:27:50Z
dc.type.es_CO.fl_str_mv	Trabajo de grado - Pregrado
dc.type.driver.none.fl_str_mv	info:eu-repo/semantics/bachelorThesis
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dc.identifier.uri.none.fl_str_mv	http://hdl.handle.net/1992/64272
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dc.identifier.reponame.es_CO.fl_str_mv	reponame:Repositorio Institucional Séneca
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url	http://hdl.handle.net/1992/64272
identifier_str_mv	instname:Universidad de los Andes reponame:Repositorio Institucional Séneca repourl:https://repositorio.uniandes.edu.co/
dc.language.iso.es_CO.fl_str_mv	eng
language	eng
dc.relation.references.es_CO.fl_str_mv	H. Beuther, R. Klessen, C. Dullemond, and T. Henning, Protostars and Planets VI, ser. The University of Arizona Space Science Series. University of Arizona Press, 2014. [Online]. Available: https://muse.jhu.edu/book/35621 K. M. Pattle, Submillimetre Studies of Prestellar and Starless Cores in the Ophi- uchus, Taurus and Cepheus Molecular Clouds. Springer, 2022. J. M. Carpenter and D. B. Sanders, "The w51 giant molecular cloud," The Astronomical Journal, vol. 116, no. 4, pp. 1856-1867, oct 1998. [Online]. Available: https://doi.org/10.1086/300534 P. André, A. Menshchikov, S. Bontemps, V. Könyves, F. Motte, N. Schneider, P. Didelon, V. Minier, P. Saraceno, D. Ward-Thompson, J. di Francesco, G. White, S. Molinari, L. Testi, A. Abergel, M. Griffin, T. Henning, P. Royer, B. Mern, R. Vavrek, M. Attard, D. Arzoumanian, C. D. Wilson, P. Ade, H. Aussel, J. P. Baluteau, M. Benedettini, J. P. Bernard, J. A. D. L. Blommaert, L. Cambrésy, P. Cox, A. di Giorgio, P. Hargrave, M. Hennemann, M. Huang, J. Kirk, O. Krause, R. Launhardt, S. Leeks, J. Le Pennec, J. Z. Li, P. G. Martin, A. Maury, G. Olofsson, A. Omont, N. Peretto, S. Pezzuto, T. Prusti, H. Roussel, D. Russeil, M. Sauvage, B. Sibthorpe, A. Sicilia-Aguilar, L. Spinoglio, C. Waelkens, A. Woodcraft, and A. Zavagno, "From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt Survey," , vol. 518, p. L102, Jul. 2010. D. Arzoumanian, P. André, P. Didelon, V. Könyves, N. Schneider, A. Menshchikov, T. Sousbie, A. Zavagno, S. Bontemps, J. di Francesco, M. Griffin, M. Hennemann, T. Hill, J. Kirk, P. Martin, V. Minier, S. Molinari, F. Motte, N. Peretto, S. Pezzuto, L. Spinoglio, D. Ward-Thompson, G. White, and C. D. Wilson," Characterizing interstellar filaments with Herschel in IC 5146 , vol. 529, p. L6, May 2011. . André, J. Di Francesco, D. Ward-Thompson, S. I. Inutsuka, R. E. Pudritz, and J. E. Pineda, "From Filamentary Networks to Dense Cores in MolecularClouds: Toward a New Paradigm for Star Formation," in Protostars and Planets VI, H. Beuther, R. S. Klessen, C. P. Dullemond, and T. Henning, Eds., Jan. 2014, p. 27. J. C. Tan, M. T. Beltrán, P. Caselli, F. Fontani, A. Fuente, M. R. Krumholz, C. F. McKee, and A. Stolte, "Massive star formation," Protostars and Planets VI, vol. 149, no. 6, 2014. F. Motte, S. Bontemps, and F. Louvet, "High-mass star and massive cluster formation in the milky way," Annual Review of Astronomy and Astrophysics, vol. 56, no. 1, pp. 41-82, 2018. [Online]. Available: https: //doi.org/10.1146/annurev-astro-091916-055235 J. C. Tan, "The birth of massive stars and star clusters," in Cores to Clusters, M. S. N. Kumar, M. Tafalla, and P. Caselli, Eds. New York, NY: Springer New York, 2005, pp. 87-104. M. R. Krumholz and C. F. McKee, "A General Theory of Turbulence-regulated Star Formation, from Spirals to Ultraluminous Infrared Galaxies," , vol. 630, no. 1, pp. 250-268, Sep. 2005. S. Van Loo, J. C. Tan, and S. A. E. G. Falle, "Magnetic Fields and Galactic Star Formation Rates," , vol. 800, no. 1, p. L11, Feb. 2015. M.-M. Mac Low and R. S. Klessen, "Control of star formation by supersonic turbulence," Rev. Mod. Phys., vol. 76, pp. 125-194, Jan 2004. [Online]. Available: https://link.aps.org/doi/10.1103/RevModPhys.76.125 B. G. Elmegreen and C. J. Lada, "Sequential formation of subgroups in OB associations." , vol. 214, pp. 725-741, Jun. 1977. A. Whitworth and N. Francis, "A threshold for sequentially self-propagating star formation," Monthly Notices of the Royal Astronomical Society, vol. 329, no. 3, pp. 641-646, 01 2002. [Online]. Available: https://doi.org/10.1046/j.1365-8711.2002. 05048.x J. C. Tan, "Star Formation Rates in Disk Galaxies and Circumnuclear Starbursts from Cloud Collisions," , vol. 536, no. 1, pp. 173-184, Jun. 2000. B. Wu, S. Van Loo, J. C. Tan, and S. Bruderer, "GMC Collisions as Triggers of Star Formation. I. Parameter Space Exploration with 2D Simulations," , vol. 811, no. 1, p. 56, Sep. 2015 S. Fujita, K. Torii, N. Kuno, A. Nishimura, T. Umemoto, T. Minamidani, M. Kohno, M. Yamagishi, T. Tosaki, M. Matsuo, Y. Tsuda, R. Enokiya, K. Tachi- hara, A. Ohama, H. Sano, K. Okawa, K. Hayashi, S. Yoshiike, D. Tsutsumi, and o. F. m. Fukui, Yasuo, "Massive star formation in W51 A triggered by cloud-cloud collisions," Publications of the Astronomical Society of Japan, vol. 73, no. Supplement 1, pp. S172-S200, 04 2019. Y. Fukui, A. Ohama, N. Hanaoka, N. Furukawa, K. Torii, J. R. Dawson, N. Mizuno, K. Hasegawa, T. Fukuda, S. Soga, N. Moribe, Y. Kuroda, T. Hayakawa, A. Kawamura, T. Kuwahara, H. Yamamoto, T. Okuda, T. Onishi, H. Maezawa, and A. Mizuno, "Molecular Clouds toward the Super Star Cluster NGC 3603 Possible Evidence for a Cloud-Cloud Collision in Triggering the Cluster Formation,". vol. 780, no. 1, p. 36, Jan. 2014. E. Moser, M. Liu, J. C. Tan, W. Lim, Y. Zhang, and J. P. Farias, "The High-mass Protostellar Population of a Massive Infrared Dark Cloud," , vol. 897, no. 2, p. 136, Jul. 2020 P. Sanhueza, Y. Contreras, B. Wu, J. M. Jackson, A. E. Guzmán, Q. Zhang, S. Li, X. Lu, A. Silva, N. Izumi, T. Liu, R. E. Miura, K. Tatematsu, T. Sakai, H. Beuther, G. Garay, S. Ohashi, M. Saito, F. Nakamura, K. Saigo, V. S. Veena, Q. Nguyen- Luong, and D. Tafoya, "The ALMA Survey of 70 "m Dark High-mass Clumps in Early Stages (ASHES). I. Pilot Survey: Clump Fragmentation," , vol. 886, no. 2, p. 102, Dec. 2019. B. Wu, J. C. Tan, D. Christie, and F. Nakamura, "GMC Collisions as Triggers of Star Formation. VII. The Effect of Magnetic Field Strength on Star Formation,", vol. 891, no. 2, p. 168, Mar. 2020. Y. Cheng, J. C. Tan, M. Liu, S. Kong, W. Lim, M. Andersen, and N. D. Rio, "The core mass function in the massive protocluster g286.210.17 revealed by ALMA," The Astrophysical Journal, vol. 853, no. 2, p. 160, feb 2018. [Online]. Available: https://doi.org/10.3847/1538-4357/aaa3f1 S. K. Balfour, A. P. Whitworth, and D. A. Hubber, "Star formation triggered by non-head-on cloud-cloud collisions, and clouds with pre-collision sub-structure," vol. 465, no. 3, pp. 3483-3494, Mar. 2017 E. Rosolowsky, J. Pineda, J. Kauffmann, and A. Goodman, "Structural analysis of molecular clouds: dendrograms," The Astrophysical Journal, vol. 679, no. 2, p. 1338, 2008. J. D. Barrow, trees, S. P. Bhavsar, and D. H. Sonoda, filaments and galaxy clustering, "Minimal spanning Monthly Notices of the Royal Astronomical Society, vol. 216, no. 1, pp. 17-35, 09 1985. [Online]. Available: https://doi.org/10.1093/mnras/216.1.17 P. Virtanen, R. Gommers, T. E. Oliphant, M. Haberland, T. Reddy, D. Cournapeau, E. Burovski, P. Peterson, W. Weckesser, J. Bright, S. J. van der Walt, M. Brett, J. Wilson, K. J. Millman, N. Mayorov, A. R. J. Nelson, E. Jones, R. Kern, E. Larson, C. J. Carey, ". Polat, Y. Feng, E. W. Moore, J. VanderPlas, D. Laxalde, J. Perktold, R. Cimrman, I. Henriksen, E. A. Quintero, C. R. Harris, A. M. Archibald, A. H. Ribeiro, F. Pedregosa, P. van Mulbregt, and SciPy 1.0 Contributors, "SciPy 1.0: Fundamental Algorithms for Scientific Computing in Python," Nature Methods, vol. 17, pp. 261-272, 2020. J. B. Kruskal, "On the shortest spanning subtree of a graph and the traveling salesman problem," Proceedings of the American Mathematical Society, vol. 7, no. 1, pp. 485050, 1956. [Online]. Available: http://www.jstor.org/stable/2033241 B. Wu, J. C. Tan, F. Nakamura, S. Van Loo, D. Christie, and D. Collins, "GMC Collisions as Triggers of Star Formation. II. 3D Turbulent, Magnetized Simulations,", vol. 835, no. 2, p. 137, Feb. 2017. D. Christie, B. Wu, and J. C. Tan, "GMC Collisions as Triggers of Star Formation. IV. The Role of Ambipolar Diffusion, , vol. 848, no. 1, p. 50, Oct. 2017. D. C. Collins, H. Xu, M. L. Norman, H. Li, and S. Li, "Cosmological Adaptive Mesh Refinement Magnetohydrodynamics with Enzo," , vol. 186, no. 2, pp. 308-333, Feb. 2010. CASA Team, B. Bean, S. Bhatnagar, S. Castro, J. Donovan Meyer, B. Emonts, E. Garcia, R. Garwood, K. Golap, J. G. Villalba, P. Harris, Y. Hayashi, J. Hoskins, M. Hsieh, P. Jagannathan, W. Kawasaki, A. Keimpema, M. Kettenis, J. Lopez, J. Marvil, J. Masters, A. McNichols, D. Mehringer, R. Miel, G. Moellenbrock, F. Montesino, T. Nakazato, J. Ott, D. Petry, M. Pokorny, R. Raba, U. Rau, D. Schiebel, N. Schweighart, S. Sekhar, K. Shimada, D. Small, J.-W. Steeb, K. Sugimoto, V. Suoranta, T. Tsutsumi, I. M. van Bemmel, M. Verkouter, A. Wells, W. Xiong, A. Szomoru, M. Griffith, B. Glendenning, and J. Kern, "CASA, the Common Astronomy Software Applications for Radio Astronomy," , vol. 134, no. 1041, p. 114501, Nov. 2022. Roy, A., André, Ph., Arzoumanian, D., Peretto, N., Palmeirim, P., Könyves, V., Schneider, N., Benedettini, M., Di Francesco, J., Elia, D., Hill, T., Ladjelate, B., Louvet, F., Motte, F., Pezzuto, S., Schisano, E., Shimajiri, Y., Spinoglio, L., Ward-Thompson, D., and White, G., "Possible link between the power spectrum of interstellar filaments and the origin of the prestellar core mass function,". A&A, vol. 584, p. A111, 2015. [Online]. Available: https://doi.org/10.1051/0004-6361/201526431 A. Cartwright and A. P. Whitworth, "The statistical analysis of star clusters," vol. 348, no. 2, pp. 589-598, Feb. 2004 R. J. Allison, S. P. Goodwin, R. J. Parker, S. F. Portegies Zwart, R. De Grijs, and M. B. N. Kouwenhoven, "Using the minimum spanning tree to trace mass segregation," Monthly Notices of the Royal Astronomical Society, vol. 395, no. 3, pp. 1449-1454, https://doi.org/10.1111/j.1365-2966.2009.14508.x
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dc.format.extent.es_CO.fl_str_mv	37 páginas
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dc.publisher.es_CO.fl_str_mv	Universidad de los Andes
dc.publisher.program.es_CO.fl_str_mv	Física
dc.publisher.faculty.es_CO.fl_str_mv	Facultad de Ciencias
dc.publisher.department.es_CO.fl_str_mv	Departamento de Física
institution	Universidad de los Andes
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spelling	Attribution-NonCommercial-NoDerivatives 4.0 Internacionalhttp://creativecommons.org/licenses/by-nc-nd/4.0/info:eu-repo/semantics/openAccesshttp://purl.org/coar/access_right/c_abf2Tan, Jonathana5d9c2d4-1192-4794-baaa-2ec16583f28f600Forero Romero, Jaime Ernestovirtual::7445-1García Alvarado, María Valentina74edf94d-3dd8-4f10-9664-83457e4c0c82600García Varela, José Alejandro2023-01-27T16:27:50Z2023-01-27T16:27:50Z2022-12-15http://hdl.handle.net/1992/64272instname:Universidad de los Andesreponame:Repositorio Institucional Sénecarepourl:https://repositorio.uniandes.edu.co/Este proyecto inició como parte de Chalmers Astrophysics & Space Science Summer (CASSUM) Research FellowshipThe main processes that trigger the collapse and fragmentation of giant molecular clouds (GMCs) in star-forming regions are poorly understood. One of the proposed mechanisms for the formation of massive stellar clusters is the collision between GMCs. In this degree project, the main objective is to study the characteristics of proto-stellar clusters formed from the simulation of the collision of two GMCs with different initial velocities and immersed in regions with different magnetic field strengths of the order of 10 - 50 microG. An introduction to the formation of star clusters in molecular clouds and some of the methods used in the development of the analysis are given in chapter 1. Simulations of the collision of giant molecular clouds used in the analysis are described in chapter 2. The filtering made, equivalent to that resulting when a structure is observed by ALMA is described in chapter 3. Subsequently, the structural analysis and protoclusters properties are presented in chapter 4. Finally, chapter 5 discusses the conclusions of the degree project and some perspectives for future work in this line of research. As a major result of this work, we found it is possible to distinguish between the collision nature of the clouds, that is, whether they collide powered by an initial velocity or purely by gravity. Some metrics presented used are able to show a correlation with magnetic field strengths for both collision cases. Some others, like filament bending angle and mass segregation fraction, work only for colliding clouds.Chalmers Astrophysics & Space Science Summer (CASSUM) Research FellowshipFísicoPregradoAstronomía37 páginasapplication/pdfengUniversidad de los AndesFísicaFacultad de CienciasDepartamento de FísicaStructural analysis of massive protoclusters formed from cloud collisionTrabajo de grado - Pregradoinfo:eu-repo/semantics/bachelorThesisinfo:eu-repo/semantics/acceptedVersionhttp://purl.org/coar/resource_type/c_7a1fTexthttp://purl.org/redcol/resource_type/TPFormación estelarNubes moleculares gigantesCampo magnéticoSimulacionesColisiónFísicaH. Beuther, R. Klessen, C. Dullemond, and T. Henning, Protostars and Planets VI, ser. The University of Arizona Space Science Series. University of Arizona Press, 2014. [Online]. Available: https://muse.jhu.edu/book/35621K. M. Pattle, Submillimetre Studies of Prestellar and Starless Cores in the Ophi- uchus, Taurus and Cepheus Molecular Clouds. Springer, 2022.J. M. Carpenter and D. B. Sanders, "The w51 giant molecular cloud," The Astronomical Journal, vol. 116, no. 4, pp. 1856-1867, oct 1998. [Online]. Available: https://doi.org/10.1086/300534P. André, A. Menshchikov, S. Bontemps, V. Könyves, F. Motte, N. Schneider, P. Didelon, V. Minier, P. Saraceno, D. Ward-Thompson, J. di Francesco, G. White, S. Molinari, L. Testi, A. Abergel, M. Griffin, T. Henning, P. Royer, B. Mern, R. Vavrek, M. Attard, D. Arzoumanian, C. D. Wilson, P. Ade, H. Aussel, J. P. Baluteau, M. Benedettini, J. P. Bernard, J. A. D. L. Blommaert, L. Cambrésy, P. Cox, A. di Giorgio, P. Hargrave, M. Hennemann, M. Huang, J. Kirk, O. Krause, R. Launhardt, S. Leeks, J. Le Pennec, J. Z. Li, P. G. Martin, A. Maury, G. Olofsson, A. Omont, N. Peretto, S. Pezzuto, T. Prusti, H. Roussel, D. Russeil, M. Sauvage, B. Sibthorpe, A. Sicilia-Aguilar, L. Spinoglio, C. Waelkens, A. Woodcraft, and A. Zavagno, "From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt Survey," , vol. 518, p. L102, Jul. 2010.D. Arzoumanian, P. André, P. Didelon, V. Könyves, N. Schneider, A. Menshchikov, T. Sousbie, A. Zavagno, S. Bontemps, J. di Francesco, M. Griffin, M. Hennemann, T. Hill, J. Kirk, P. Martin, V. Minier, S. Molinari, F. Motte, N. Peretto, S. Pezzuto, L. Spinoglio, D. Ward-Thompson, G. White, and C. D. Wilson," Characterizing interstellar filaments with Herschel in IC 5146 , vol. 529, p. L6, May 2011.. André, J. Di Francesco, D. Ward-Thompson, S. I. Inutsuka, R. E. Pudritz, and J. E. Pineda, "From Filamentary Networks to Dense Cores in MolecularClouds: Toward a New Paradigm for Star Formation," in Protostars and Planets VI, H. Beuther, R. S. Klessen, C. P. Dullemond, and T. Henning, Eds., Jan. 2014, p. 27.J. C. Tan, M. T. Beltrán, P. Caselli, F. Fontani, A. Fuente, M. R. Krumholz, C. F. McKee, and A. Stolte, "Massive star formation," Protostars and Planets VI, vol. 149, no. 6, 2014.F. Motte, S. Bontemps, and F. Louvet, "High-mass star and massive cluster formation in the milky way," Annual Review of Astronomy and Astrophysics, vol. 56, no. 1, pp. 41-82, 2018. [Online]. Available: https: //doi.org/10.1146/annurev-astro-091916-055235J. C. Tan, "The birth of massive stars and star clusters," in Cores to Clusters, M. S. N. Kumar, M. Tafalla, and P. Caselli, Eds. New York, NY: Springer New York, 2005, pp. 87-104.M. R. Krumholz and C. F. McKee, "A General Theory of Turbulence-regulated Star Formation, from Spirals to Ultraluminous Infrared Galaxies," , vol. 630, no. 1, pp. 250-268, Sep. 2005.S. Van Loo, J. C. Tan, and S. A. E. G. Falle, "Magnetic Fields and Galactic Star Formation Rates," , vol. 800, no. 1, p. L11, Feb. 2015.M.-M. Mac Low and R. S. Klessen, "Control of star formation by supersonic turbulence," Rev. Mod. Phys., vol. 76, pp. 125-194, Jan 2004. [Online]. Available: https://link.aps.org/doi/10.1103/RevModPhys.76.125B. G. Elmegreen and C. J. Lada, "Sequential formation of subgroups in OB associations." , vol. 214, pp. 725-741, Jun. 1977.A. Whitworth and N. Francis, "A threshold for sequentially self-propagating star formation," Monthly Notices of the Royal Astronomical Society, vol. 329, no. 3, pp. 641-646, 01 2002. [Online]. Available: https://doi.org/10.1046/j.1365-8711.2002. 05048.xJ. C. 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Kouwenhoven, "Using the minimum spanning tree to trace mass segregation," Monthly Notices of the Royal Astronomical Society, vol. 395, no. 3, pp. 1449-1454, https://doi.org/10.1111/j.1365-2966.2009.14508.x201813544Publicationhttps://scholar.google.es/citations?user=TLTK6WgAAAAJvirtual::7445-10000-0002-2890-3725virtual::7445-1https://scienti.minciencias.gov.co/cvlac/visualizador/generarCurriculoCv.do?cod_rh=0000337102virtual::7445-1d34cd5a0-50f5-42ea-825e-b51f5368f321virtual::7445-1d34cd5a0-50f5-42ea-825e-b51f5368f321virtual::7445-1CC-LICENSElicense_rdflicense_rdfapplication/rdf+xml; charset=utf-8805https://repositorio.uniandes.edu.co/bitstreams/044d2baa-e676-4ec4-9daa-695bd190e940/download4460e5956bc1d1639be9ae6146a50347MD52ORIGINALTesis_.pdfTesis_.pdfTrabajo de gradoapplication/pdf10006042https://repositorio.uniandes.edu.co/bitstreams/9c079222-8769-4dfc-9375-f3acca42c12a/downloadebba54754313aa0e9cdb3d406a8f5beeMD54093f8a4d-ddc8-4528-9179-b78a09426111.pdf093f8a4d-ddc8-4528-9179-b78a09426111.pdfHIDEapplication/pdf189532https://repositorio.uniandes.edu.co/bitstreams/e45d5b47-f741-40c2-9b04-d93d51f47e4e/download9c6e7bb4e4bd2ef8ab95ddffa14e0354MD55LICENSElicense.txtlicense.txttext/plain; charset=utf-81810https://repositorio.uniandes.edu.co/bitstreams/d9354eb7-2c1f-499e-bf32-45fb0409dd4f/download5aa5c691a1ffe97abd12c2966efcb8d6MD53THUMBNAILTesis_.pdf.jpgTesis_.pdf.jpgIM Thumbnailimage/jpeg8485https://repositorio.uniandes.edu.co/bitstreams/a89e1340-7f53-47e7-bf5f-8dc66d07c908/downloada9864e2fe53b96cc506db4f1c783a72fMD57093f8a4d-ddc8-4528-9179-b78a09426111.pdf.jpg093f8a4d-ddc8-4528-9179-b78a09426111.pdf.jpgIM Thumbnailimage/jpeg16059https://repositorio.uniandes.edu.co/bitstreams/630c593b-3627-4634-8144-c2a916473354/download9194c1090f1cde5812502156c709f355MD59TEXTTesis_.pdf.txtTesis_.pdf.txtExtracted texttext/plain68117https://repositorio.uniandes.edu.co/bitstreams/a90eeaa4-813a-4008-b9d2-36dd49a1f431/download6bb42f92bc4e243e0fb1cfe7f4f471b4MD56093f8a4d-ddc8-4528-9179-b78a09426111.pdf.txt093f8a4d-ddc8-4528-9179-b78a09426111.pdf.txtExtracted texttext/plain1163https://repositorio.uniandes.edu.co/bitstreams/c9859b2c-c8c8-4968-a5a4-7134ae562527/download4491fe1afb58beaaef41a73cf7ff2e27MD581992/64272oai:repositorio.uniandes.edu.co:1992/642722024-03-13 13:26:06.292http://creativecommons.org/licenses/by-nc-nd/4.0/open.accesshttps://repositorio.uniandes.edu.coRepositorio institucional Sénecaadminrepositorio@uniandes.edu.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

Structural analysis of massive protoclusters formed from cloud collision

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