The 0.1-2.5 keV X-ray spectrum of the O4f star ζ Puppis
- Author
- HILLIER, D. J1 ; KUDRITZKI, R. P1 ; PAULDRACH, A. W1 ; BAADE, D; CASSINELLI, J. P; PULS, J1 ; SCHMITT, J. H. M. M
[1] Inst. Astronomie astrophysik, W-8000 München, Germany - Source
Astronomy and astrophysics (Berlin. Print). 1993, Vol 276, Num 1, pp 117-128 ; ref : 53 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
- Keyword (fr)
- Ajustement modèle Emission RX Etoile O Etoile premier type Observation par satellite Perte masse Spectre RX Supergéante Vent stellaire Satellite ROSAT ζ Pup
- Keyword (en)
- Model matching X ray emission O star First type star Satellite observation Mass loss X ray spectrum Supergiant Stellar wind
- Keyword (es)
- Ajustamiento modelo Emisión RX Estrella O Estrella primer tipo Observación por satélite Pérdida masa Espectro RX Supergigante Viento estelar
- Classification
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C20 Normal stars (by class): general or individual / 001E03C20P Supergiant stars
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 4877105
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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