Near-IR features in late type stars: their relation with stellar atmosphere parameters
- Author
- DIAZ, A. I1 ; TERLEVICH, E; TERLEVICH, R
[1] Univ. autónoma Madrid, dep. física teórica, Madrid 28049, Spain - Source
Monthly Notices of the Royal Astronomical Society. 1989, Vol 239, Num 2, pp 325-345 ; ref : 20 ref
- CODEN
- MNRAA4
- ISSN
- 0035-8711
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- Blackwell Science, Oxford
- Publication country
- United Kingdom
- Document type
- Article
- Language
- English
- Keyword (fr)
- Amas globulaire Analyse composante principale Atmosphère stellaire Calcium Etoile type avancé Gravité Magnésium Métallicité Observation spectroscopique Raie absorption Raie spectrale Spectre IR proche Température effective Force raie Spectrométrie CCD
- Keyword (en)
- Globular cluster Principal component analysis Stellar atmosphere Calcium Late type star Gravity Magnesium Metallicity Spectroscopical observation Absorption line Spectral line Near infrared spectrum Effective temperature
- Keyword (es)
- Cúmulo globular Análisis componente principal Atmósfera estelar Calcio Estrella tipo avanzada Gravedad Magnesio Metalicidad Observación espectroscópica Raya absorción Raya espectral Espectro IR próximo Temperatura efectiva
- Classification
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C10 Stellar characteristics and properties / 001E03C10E Stellar atmospheres (photospheres, chromospheres, coronae, magnetospheres). Radiative transfer. Opacity and line formation
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 6572467
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
10.1093/mnras/239.2.325 
https://dx.doi.org/10.1093/mnras/239.2.325
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