HIGH-RESOLUTION OBSERVATIONS OF MOLECULAR LINES TOWARD THE HOT CORE G28.20-0.04N
- Author
- QIN, Sheng-Li1 ; MAOHAI HUANG1 ; YUEFANG WU2 ; RUI XUE1 ; SHENG CHEN1
[1] National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
[2] Department of Astronomy, Peking University, Beijing 100871, China - Source
The Astrophysical journal. 2008, Vol 686, Num 1 ; L21-L24 ; 2 ; ref : 1/4 p
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- University of Chicago Press, Chicago, IL
- Publication country
- United States
- Document type
- Article
- Language
- English
- Author keyword
- H II regions-ISM: individual (G28.20-0.04N)-ISM: kinematics and dynamics ISM: molecules radio lines: ISM-stars: formation
- Keyword (fr)
- Cinématique Dynamique Etoile radio Formation raie Formation stellaire Région HII
- Keyword (en)
- Kinematics Dynamics Radio stars Line formation Star formation HII regions
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20747128
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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DOI
10.1086/592785 
https://dx.doi.org/10.1086/592785
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