Infrared detection of gas phase formaldehyde towards the high mass protostar W33A
- Author
- ROUEFF, E1 ; DARTOIS, E2 ; GEBALLE, T. R3 ; GERIN, M4
[1] Laboratoire Univers et Théorie, UMR 8102 du CNRS, Observatoire de Paris, Section de Meudon, Place Jules Janssen, 92195 Meudon, France
[2] IAS, Bat. 121, Université Paris Sud, 91405 Orsay, France
[3] Gemini Observatory, 670 N. A'ohoku Place, Hilo, HI 96720, United States
[4] Laboratoire d'Étude du Rayonnement et de la Matière en Astrophysique, UMR 8112 du CNRS, Observatoire de Paris and École Normale Supérieure, 24 rue Lhomond, 75231 Paris, France - Source
Astronomy and astrophysics (Berlin. Print). 2006, Vol 447, Num 3, pp 963-969, 7 p ; ref : 44 ref
- CODEN
- AAEJAF
- ISSN
- 0004-6361
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- EDP Sciences, Les Ulis
- Publication country
- France
- Document type
- Article
- Language
- English
- Author keyword
- ISM: molecules molecular processes stars: circumstellar matter stars: formation
- Keyword (fr)
- Abondance Borne supérieure Continuum Densité colonne Détection IR Evaporation Formaldéhyde Formation stellaire Matière circumstellaire Mécanisme formation Nuage interstellaire Photodissociation Processus moléculaire Proto étoile Raie absorption Sublimation
- Keyword (en)
- Abundance Upper bound Continuum Column density Infrared detection Evaporation Formaldehyde Star formation Circumstellar matter Formation mechanism Interstellar clouds Photodissociation Molecular process Protostars Absorption line Sublimation
- Keyword (es)
- Cota superior Continuo Densidad columna Detección IR Mecanismo formacion Proceso molecular Raya absorción
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 17482242
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
10.1051/0004-6361:20053639 
https://dx.doi.org/10.1051/0004-6361:20053639
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