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 (US) |
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Title of host publication | MAGNETIC FIELDS IN THE UNIVERSE |
Subtitle of host publication | From Laboratory and Stars to Primordial Structures |
Pages | 140-144 |
Number of pages | 5 |
Volume | 784 |
DOIs | |
State | Published - Sep 28 2005 |
Externally published | Yes |
Event | MAGNETIC FIELDS IN THE UNIVERSE: From Laboratory and Stars to Primordial Structures - Angra dos Reis, Brazil Duration: Nov 28 2004 → Dec 3 2004 |
Other
Other | MAGNETIC FIELDS IN THE UNIVERSE: From Laboratory and Stars to Primordial Structures |
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Country/Territory | Brazil |
City | Angra dos Reis |
Period | 11/28/04 → 12/3/04 |
Keywords
- Star Formation
ASJC Scopus subject areas
- Physics and Astronomy(all)