Cometary water expansion velocity from OH line shapes
- Author
- TSENG, W.-L1 2 ; BOCKELEE-MORVAN, D1 ; CROVISIER, J1 ; COLOM, P1 ; IP, W.-H2
[1] Observatoire de Paris, 5 place Jules Janssen, 92195 Meudon, France
[2] Institute of Astronomy, National Central University, Chung Li 32054, Taiwan, Province of China - Source
Astronomy and astrophysics (Berlin. Print). 2007, Vol 467, Num 2, pp 729-735, 7 p ; ref : 1/4 p
- 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
- comets: general line: profiles molecular processes radio lines: solar system
- Keyword (fr)
- Comète Distance héliocentrique Modèle atmosphère Modèle hydrodynamique Processus moléculaire Profil raie Radical hydroxyle Système solaire Taux production Vitesse expansion
- Keyword (en)
- Comets Heliocentric distance Atmosphere model Hydrodynamic model Molecular process Line shape Hydroxyl radicals Solar system Production rate Expansion velocity
- Keyword (es)
- Distancia heliocéntrica Modelo atmósfera Proceso molecular Índice producción Velocidad expansión
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 18743313
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
10.1051/0004-6361:20066666 
https://dx.doi.org/10.1051/0004-6361:20066666
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