Soft X-ray emissions of highly charged Si VII-Si XII in cool star -Procyon
- Author
- LIANG, G. Y1 ; ZHAO, G1
[1] National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China - Source
Monthly Notices of the Royal Astronomical Society. 2008, Vol 384, Num 2, pp 489-496, 8 p ; ref : 1/2 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
- X-rays: general line: identification methods: analytical stars: coronae
- Keyword (fr)
- Couronne stellaire Emission RX Eruption solaire Etoile froide Identification raie Loi normale Mesure émission Méthode analytique Raie émission Rayon X mou Soleil
- Keyword (en)
- Stellar coronae X ray emission Solar flares Cool star Line identification Normal distribution Emission measure Analytical method Emission line Soft X radiation Sun
- Keyword (es)
- Emisión RX Estrella fría Identificación raya Medida emisión Método analítico Raya emisión
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20144389
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
10.1111/j.1365-2966.2007.12696.x 
https://dx.doi.org/10.1111/j.1365-2966.2007.12696.x
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