Orion B (NGC 2024). III: BIMA SO Jk=22→11 observations : evidence for peculiar sulfur chemistry
- Author
- BARNES, P. J1 ; CRUTCHER, R. M
[1] Univ. Toronto, canadian inst. theoritical astrophysics, McLennan physical laboratories, Toronta ON M5S 1A1, Canada - Source
The Astrophysical journal. 1992, Vol 389, Num 1, pp 325-337 ; p.1 ; ref : 32 ref
- 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
- Keyword (fr)
- Carte radio Molécule interstellaire Nuage moléculaire Observation radio Région formation stellaire Soufre oxyde Structure NGC 2024 Ori B
- Keyword (en)
- Radio map Interstellar molecule Molecular cloud Radio observation Stellar formation region Sulfur oxide Structure
- Keyword (es)
- Mapa radio Molécula interestelar Nube molecular Observación radio Región formación estelar Azufre óxido Estructura
- Classification
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D38 Interstellar medium (ism) and nebulae in milky way / 001E03D38D Molecular clouds, h2 clouds, dense clouds, and dark clouds
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 5197258
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
10.1086/171207 
https://dx.doi.org/10.1086/171207
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