The B-type giant HD 271791 in the Galactic halo : Linking run-away stars to hyper-velocity stars
- Author
- HEBER, U1 ; EDELMANN, H1 ; NAPIWOTZKI, R2 ; ALTMANN, M3 ; SCHOLZ, R.-D4
[1] Dr. Remeis-Sternwarte, Astronomisches Institut der Universität Erlangen-Nürnberg, Sternwartstr. 7, 96049 Bamberg, Germany
[2] Centre for Astrophysics Research, University of Hertfordshire, College Lane, Hatfield AL10 9AB, United Kingdom
[3] ARI, Zentrum für Astronomie der Universität Heidelberg, Mönchhofstr. 12-14, 69120 Heidelberg, Germany
[4] Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany - Source
Astronomy and astrophysics (Berlin. Print). 2008, Vol 483, Num 2 ; L21-L24 ; 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: center Galaxy: halo stars: atmospheres stars: distances stars: early-type stars: individual: HD 271791
- Keyword (fr)
- Centre galactique Cinématique Composition chimique Cosmologie Disque galactique Espace vitesse Etoile B Etoile jeune Etoile massive Etoile premier type Etoile rotation Galaxies Halo galactique Halo galaxies Modèle atmosphère Mouvement propre Rotation rapide Simulation numérique Soleil Spectre optique Trou noir supermassif Vitesse fuite Voie lactée
- Keyword (en)
- Galactic centers Kinematics Chemical composition Cosmology Galactic disks Velocity space B stars Young stars Massive stars Early type stars Rotating star Galaxies Galactic halos Galaxy halo Atmosphere model Proper motion Rapid rotation Digital simulation Sun Optical spectrum Supermassive black hole Escape velocity Milky Way
- Keyword (es)
- Espacio velocidad Estrella rotación Halo galaxia Modelo atmósfera Rotación rápida Espectro óptico Agujero negro supermasivo
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20358072
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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