Star Formation Histories

Thibaut Lery, Celine Combet, Gareth Murphy

Research output: Chapter in Book/Report/Conference proceedingArticle in proceedingsResearchpeer-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
Title of host publicationMagnetic Fields in the Universe: From Laboratory and Stars to Primordial Structures.
EditorsE. M. de Gouveia Dal Pino, G. Lugones, A. Lazarian
Volume784
Publication date2005
Pages140-144
DOIs
Publication statusPublished - 2005
Externally publishedYes
EventMagnetic Fields in the Universe: From Laboratory and Stars to Primordial Structures. - Angra dos Reis, Brazil
Duration: 28 Nov 20143 Dec 2014

Conference

ConferenceMagnetic Fields in the Universe: From Laboratory and Stars to Primordial Structures.
CountryBrazil
CityAngra dos Reis
Period28/11/201403/12/2014

Keywords

  • Star formation

Fingerprint Dive into the research topics of 'Star Formation Histories'. Together they form a unique fingerprint.

Cite this