SiO emission as a tracer of shocked gas in molecular outflows
- Autor
- MARTIN-PINTADO, J; BACHILLER, R; FUENTE, A
Cent. astronómico Yebes, 19080 Guadalajara, Spain - Fuente
Astronomy and astrophysics (Berlin. Print). 1992, Vol 254, Num 1-2, pp 315-326 ; ref : 41 ref
- CODEN
- AAEJAF
- ISSN
- 0004-6361
- Campo Científico
- Astronomy earth cosmic environment
- Editor
- EDP Sciences, Les Ulis
- País de la publicación
- France
- Tipo de documento
- Article
- Idioma
- English
- Palabra clave (fr)
- Abondance Densité colonne Ecoulement moléculaire Emission Formaldéhyde Hydrogène Cyanure Ion positif Molécule interstellaire Observation radio Paramètre physique Profil raie spectrale Silicium Oxyde Soufre oxyde Table donnée Vent stellaire B 1 Cep A L 1448 NGC 2071
- Palabra clave (in)
- Abundance Column density Molecular flow Emission Formaldehyde Hydrogen Cyanides Positive ion Interstellar molecule Radio observation Physical parameter Spectral line profile Silicon Oxides Sulfur oxide Data table Stellar wind
- Palabra clave (es)
- Abundancia Densidad columna Flujo molecular Emisión Formaldehído Hidrógeno Cianuro Ión positivo Molécula interestelar Observación radio Parámetro físico Perfil raya espectral Silicio Óxido Azufre óxido Tabla dato Viento estelar
- Clasificación
- 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
- Disciplina
- Astronomy
- Procedencia
- Inist-CNRS
- Base de datos
- PASCAL
- Identificador INIST
- 5066851
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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