The X-ray luminosity of solar-mass stars in the intermediate age open cluster NGC 752
- Author
- GIARDINO, G1 ; PILLITTERI, I2 ; FAVATA, F3 ; MICELA, G4
[1] ESA -Research and Science Support Department, ESTEC, Postbus 299, 2200 AG Noordwijk, Netherlands
[2] DSFA, Università degli Studi di Palermo, Piazza del Parlamento 1, 90134 Palermo, Italy
[3] ESA -Planning and Community Coordination Office, Science Programme, 8-10 rue Mario Nikis, 75738 Paris, France
[4] INAF -Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134 Palermo, Italy - Source
Astronomy and astrophysics (Berlin. Print). 2008, Vol 490, Num 1, pp 113-123, 11 p ; ref : 1/4 p
- CODEN
- AAEJAF
- ISSN
- 0004-6361
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- EDP Sciences, Les Ulis
- Publication country
- France
- Document type
- Article
- Language
- English
- Author keyword
- Galaxy: open clusters and associations: individual: NGC 752 X-rays: stars stars: coronae stars: rotation
- Keyword (fr)
- Age Amas galaxies Amas ouvert Amas stellaire Couronne stellaire Emission RX Etoile S Etoile membre Evolution stellaire Luminosité Masse stellaire Pléiades Rotation stellaire Soleil Structure interne stellaire Vitesse rotation
- Keyword (en)
- Age Galaxy clusters Open clusters Star clusters Stellar coronae X ray emission S stars Member star Stellar evolution Luminosity Stellar mass Pleiades Stellar rotation Sun Stellar interiors Rotation speed
- Keyword (es)
- Edad Emisión RX Estrella miembro Velocidad rotación
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20751942
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
10.1051/0004-6361:200810042 
https://dx.doi.org/10.1051/0004-6361:200810042
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