Pascal and Francis Bibliographic Databases

Help

Export

Selection :

Permanent link
http://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=22314312

12.2-GHz methanol masers towards 1.2-mm dust clumps: quantifying high-mass star formation evolutionary schemes

Author
BREEN, S. L1 2 ; ELLINGSEN, S. P1 ; CASWELL, J. L2 ; LEWIS, B. E1
[1] School of Mathematics and Physics, University of Tasmania, Private Bag 37, Hobart, Tasmania 7001, Australia
[2] Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 1710, Australia
Source

Monthly notices of the Royal Astronomical Society (Print). 2010, Vol 401, Num 4, pp 2219-2244, 26 p ; ref : 3/4 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: molecules masers radio lines: ISM stars: formation
Keyword (fr)
Continuum Couleur Densité flux Densité élevée Durée vie Etoile massive Etude IR Formation stellaire Luminosité Maser Masse stellaire Méthanol Région formation stellaire Source ponctuelle Sous groupe
Keyword (en)
Continuum Color Flux density High density Lifetime Massive stars Infrared surveys Star formation Luminosity Masers Stellar mass Methanol Stellar formation region Point sources Subgroup
Keyword (es)
Continuo Densidad elevada Región formación estelar Subgrupo
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
22314312

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

Access to the document

Searching the Web