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...
保存先:
| 出版年: | Revista Mexicana de Astronomía y Astrofísica |
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| 第一著者: | |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
Universidad Nacional Autónoma de México
2016
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| 主題: | |
| オンライン･アクセス: | https://www.redalyc.org/articulo.oa?id=57146052012 |
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