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Forming protostars in molecular clouds with shocked envelope expansion and core collapse

Author
LOU, Yu-Qing1 2 3 ; YANG GAO1
[1] Department of Physics and Tsinghua Centre for Astrophysics (THCA), Tsinghua University, Beijing 100084, China
[2] National Astronomical Observatories of China, Chinese Academy of Sciences, A20 Datun Road, Beijing 100012, China
[3] Department of Astronomy and Astrophysics, The University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, United States
Source

Monthly notices of the Royal Astronomical Society (Print). 2011, Vol 412, Num 3, pp 1755-1764, 10 p ; ref : 1/2 p

CODEN
MNRAA4
ISSN
0035-8711
Scientific domain
Astronomy earth cosmic environment
Publisher
Wiley-Blackwell, Malden, MA
Publication country
United States
Document type
Article
Language
English
Author keyword
ISM: clouds ISM: individual objects: FeSt 1-457 line: profiles outflows radiative transfer stars: formation stars: winds
Keyword (fr)
Continuum Densité colonne Dynamique Effondrement Etoile faible masse Formation stellaire Gravité Modèle Noyau stellaire Nuage moléculaire Profil raie Proto étoile Transfert radiatif Vent stellaire
Keyword (en)
Continuum Column density Dynamics Collapse Low-mass stars Star formation Gravity Models Stellar cores Molecular clouds Line shape Protostars Radiative transfer Stellar winds
Keyword (es)
Continuo Densidad columna Desmoronamiento Modelo
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
24024872

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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