The relation between surface star formation rate density and spiral arms in NGC 5236 (M 83)

ABSTRACT:Context. For a long time the consensus has been that star formation rates are higher in the interior of spiral arms in galaxies, compared to inter-arm regions. However, recent studies have found that the star formation inside the arms is not more efficient than elsewhere in the galaxy. Prev...

Full description

Autores:

Silva Villa, Esteban
Larsen, Soeren

Tipo de recurso:

Article of investigation

Fecha de publicación:

2012

Institución:

Universidad de Antioquia

Repositorio:

Repositorio UdeA

Idioma:

eng

OAI Identifier:

oai:bibliotecadigital.udea.edu.co:10495/33542

Acceso en línea:

https://hdl.handle.net/10495/33542

Palabra clave:

Galaxias
Galaxies
Estrellas - Formación
Stars - formation - congresses
NGC 5236

Rights

openAccess

License

http://creativecommons.org/licenses/by/2.5/co/