The distribution of the local interstellar medium derived from MgII column densities towards seven cool stars
- Author
- VLADILO, G1 ; BECKMAN, J. E; CRIVELLARI, L; FRANCO, M. L; MOLARO, P
[1] Osservatorio astronomico Trieste, Trieste 34131, Italy - Source
Astronomy and astrophysics (Berlin. Print). 1985, Vol 144, Num 1, pp 81-86 ; ref : 13 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)
- Etoile froide Etoile type avancé Magnésium Matière interstellaire Observation par satellite Raie absorption Table donnée 24 UMa Α Hyi Β Hyi Β TrA Δ Pav Ζ Tuc τ Cet Satellite IUE
- Keyword (en)
- Cool star Late type star Magnesium Interstellar matter Satellite observation Absorption line Data table
- Keyword (es)
- Magnesio
- 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
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 9207348
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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