THE FORMATION MASS OF A BINARY SYSTEM VIA FRAGMENTATION OF A ROTATING PARENT CORE WITH INCREASING TOTAL MASS
We present a set of numerical simulations of the gravitational collapse of a uniform and rotating core, in which azimuthal symmetric mass seeds are initially implemented in order to favor the formation of a dense filament, out of which a binary system may be formed by direct fragmentation. We observ...
Gardado en:
| Publicado en: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Autor Principal: | |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado: |
Universidad Nacional Autónoma de México
2016
|
| Assuntos: | |
| Acceso en liña: | https://www.redalyc.org/articulo.oa?id=57146052012 |
| Tags: |
Sen Etiquetas, Sexa o primeiro en etiquetar este rexistro!
|