EnglishThe paper discusses the problem of fragmentation in a rotating cloud, showing that different physical models can result in widely different results. It is also shown that results of the present 'turbulent-rotation' model agree qualitatively with those of numerical calculations by Larson (1978) and it is suggested that fragmentation in a rotating nebula takes place at two different stages.
| Autori interni: | PAOLICCHI, PAOLO |
| Autori: | Paolicchi P; Siccardi S |
| Titolo: | Two-stage fragmentation in a rotating protostellar cloud |
| Anno del prodotto: | 1979 |
| Digital Object Identifier (DOI): | 10.1007/BF00639522 |
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