Physics
Scientific paper
Sep 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..784..140l&link_type=abstract
MAGNETIC FIELDS IN THE UNIVERSE: From Laboratory and Stars to Primordial Structures. AIP Conference Proceedings, Volume 784, pp
Physics
2
Star Formation, Pre-Main-Sequence Stars, Pre-Main Sequence Objects, Young Stellar Objects And Protostars
Scientific paper
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.
Combet Céline
Lery Thibaut
Murphy Gareth
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