The four leading arms of the Magellanic Cloud system: Evidence for interaction with Milky Way disk and halo
- Author
- VENZMER, M. S1 2 ; KERP, J1 ; KALBERLA, P. M. W1
[1] Argelander-Institut für Astronomic, Auf dem Hügel 71, 53121 Bonn, Germany
[2] Institut für Astrophysik, Friedrich-Hund-Platz 1, 37077 Göttingen, Germany - Source
Astronomy and astrophysics (Berlin. Print). 2012, Vol 547 ; A12.1-A12.11 ; 1 ; 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: evolution Galaxy: halo Magellanic Clouds galaxies: interactions
- Keyword (fr)
- Algorithme Asymétrie Catalogue astronomique Corrélation Densité colonne Disque galactique Décélération Etude ciel Evolution galaxies Galaxies Grand Nuage Magellan Halo galaxies Largeur raie Nuages Magellan Profil raie Vitesse radiale Voie lactée
- Keyword (en)
- Algorithms Asymmetry Astronomical catalogues Correlations Column density Galactic disks Deceleration Sky surveys Galaxy evolution Galaxies Large Magellanic Cloud Galaxy halo Line widths Magellanic Clouds Line shape Radial velocity Milky Way
- Keyword (es)
- Densidad columna Desaceleración Evolución galaxias Halo galaxia
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 26783891
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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