An Effelsberg HI study of the ISM around WR 126, WR 154 and WR 155
- Author
- CICHOWOLSKI, S1 ; ARNAL, E. M1 2
[1] Instituto Argentino de Radioastronomía, CC # 5, 1894 Villa Elisa, Argentina
[2] Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional La Plata, 1900 La Plata, Argentina - Source
Astronomy and astrophysics (Berlin. Print). 2004, Vol 414, Num 1, pp 203-209, 7 p ; ref : 43 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: bubbles stars: Wolf-Rayet stars: individual: WR 126, WR 154, WR 155
- Keyword (fr)
- Bulle interstellaire Etoile type Wolf Rayet Hydrogène neutre Masse manquante Observation radio Raie 21 cm Raie interstellaire Région HI
- Keyword (en)
- Interstellar bubble Wolf-Rayet stars Neutral hydrogen Missing mass Radio observation 21cm-Line Interstellar line HI regions
- Keyword (es)
- Burbuja interestelar Hidrógeno neutro Observación radio Raya 21 cm Raya interestelar
- Classification
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C30 Variable and peculiar stars (including novae) / 001E03C30E Emission-line stars (of, be, luminous blue variables, wolf-rayet, etc.)
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D58 Interstellar medium (ism) and nebulae in external galaxies / 001E03D58G H i regions and 21-cm lines ; diffuse, translucent, and high-velocity clouds
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 15416454
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
10.1051/0004-6361:20031620 
https://dx.doi.org/10.1051/0004-6361:20031620
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