Abstract
The present article addresses the problem of the formation of both low and high mass stars. We suggest how competing factors change the behaviours of proto‐stellar sources and outflows in both cases. We also describe a possible temporal sequence for flows around a protostar, that may help to give a physical justification to the empirical classification of pre‐main sequence sources.
Original language | English |
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Title of host publication | Magnetic Fields in the Universe: From Laboratory and Stars to Primordial Structures. |
Editors | E. M. de Gouveia Dal Pino, G. Lugones, A. Lazarian |
Volume | 784 |
Publication date | 2005 |
Pages | 140-144 |
DOIs | |
Publication status | Published - 2005 |
Externally published | Yes |
Event | Magnetic Fields in the Universe: From Laboratory and Stars to Primordial Structures. - Angra dos Reis, Brazil Duration: 28 Nov 2014 → 3 Dec 2014 |
Conference
Conference | Magnetic Fields in the Universe: From Laboratory and Stars to Primordial Structures. |
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Country/Territory | Brazil |
City | Angra dos Reis |
Period | 28/11/2014 → 03/12/2014 |
Keywords
- Star formation