A potential new method for determining the temperature of cool stars
- Author
- VITI, S1 ; JONES, H. R. A2 ; RICHTER, M. J3 ; BARBER, R. J1 ; TENNYSON, J1 ; LACY, J. H4
[1] Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
[2] Centre for Astrophysics Research, University of Hertfordshire, College Lane, Hatfield AL10 9AB, United Kingdom
[3] Physics Department, UC Davis, One Shields Avenue, Davis, CA 95616, United States
[4] Department of Astronomy, University of Texas at Austin, 1 University Station, Austin, TX 78712, United States - Source
Monthly Notices of the Royal Astronomical Society. 2008, Vol 388, Num 3, pp 1305-1313, 9 p ; ref : 1/4 p
- CODEN
- MNRAA4
- ISSN
- 0035-8711
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- Blackwell Science, Oxford
- Publication country
- United Kingdom
- Document type
- Article
- Language
- English
- Author keyword
- infrared: stars stars: atmospheres stars: fundamental parameters stars: low-mass, brown dwarfs
- Keyword (fr)
- Etoile IR Etoile faible masse Etoile froide Naine brune Spectre IR Température effective Transition rotationnelle
- Keyword (en)
- Infrared star Low-mass stars Cool star Brown dwarf stars Infrared spectra Effective temperature Rotational transition
- Keyword (es)
- Estrella IR Estrella fría Transición rotacional
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20577608
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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