A spectroscopic investigation of η Carinae and the Homunculus Nebula. I : Overview of the spectra
- Author
- HILLIER, D. J; ALLEN, D. A
Inst. astronomy astrophysics, 8000 Munich, Germany - Source
Astronomy and astrophysics (Berlin. Print). 1992, Vol 262, Num 1, pp 153-170 ; ref : 1 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
- Keyword (fr)
- Ecoulement bipolaire Etoile raie émission Etoile variable bleue lumineuse Nébuleuse réfléchissante Observation spectroscopique Perte masse Poussière circumstellaire Profil raie spectrale Profil raie type P Cygni Rougissement interstellaire Spectre Table donnée η Car
- Keyword (en)
- Bipolar flow Emission line star Luminous blue variable star Reflecting nebula Spectroscopical observation Mass loss Circumstellar dust Spectral line profile P Cygni line profile Interstellar reddening Spectrum Data table
- Keyword (es)
- Flujo bipolar Estrella raya emisión Estrella variable azul luminosa Nebulosa reflectora Observación espectroscópica Pérdida masa Polvo circunstelar Perfil raya espectral Perfil raya tipo P Cygni Enrojecimiento interestelar Espectro Tabla dato
- 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 / 001E03D38H H ii regions. Emission and reflection nebulae
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 5512322
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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