Star formation histories

Thibaut Lery*, Celine Combet, Gareth Murphy

*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

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 languageEnglish (US)
Title of host publicationMAGNETIC FIELDS IN THE UNIVERSE
Subtitle of host publicationFrom Laboratory and Stars to Primordial Structures
Pages140-144
Number of pages5
Volume784
DOIs
StatePublished - Sep 28 2005
Externally publishedYes
EventMAGNETIC FIELDS IN THE UNIVERSE: From Laboratory and Stars to Primordial Structures - Angra dos Reis, Brazil
Duration: Nov 28 2004Dec 3 2004

Other

OtherMAGNETIC FIELDS IN THE UNIVERSE: From Laboratory and Stars to Primordial Structures
CountryBrazil
CityAngra dos Reis
Period11/28/0412/3/04

Keywords

  • Star Formation

ASJC Scopus subject areas

  • Physics and Astronomy(all)

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