A new population of extended, luminous star clusters in the halo of M31
Identifieur interne : 00A339 ( Main/Exploration ); précédent : 00A338; suivant : 00A340A new population of extended, luminous star clusters in the halo of M31
Auteurs : A. P. Huxor [Royaume-Uni] ; N. R. Tanvir ; M. J. Irwin ; R. Ibata [France] ; J. L. Collett ; A. M. N. Ferguson [Royaume-Uni] ; T. Bridges [Canada] ; G. F. Lewis [Australie]Source :
- Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2005-07.
Descripteurs français
- Pascal (Inist)
English descriptors
- KwdEn :
- Absolute magnitude, Aperture photometry, Arcsec, Bekki chiba, Bergh, Bergh mackey, Bright stars, Brodie larsen, Cluster, Color, Color-magnitude diagrams, Dsphs, Dwarf, Dwarf galaxy, Dwarf spheroidals, Galaxies, Galaxy, Galaxy clusters, Giant galaxy, Globular clusters, Halo, Hilker infante, Host galaxies, Intermediate forms, Iraf implementation, Irwin, Irwin hatzidimitriou, Irwin lewis, Isaac newton telescope, Large number, Large radii, Larsen, Lenticular galaxies, Lled points, Luminosity, Luminous star clusters, Milky Way, Mnras, Parameter space, Photometry, Progenitor dwarf, Star cluster, Star clusters, Such clusters, Super star clusters, Tidal radii, galaxies: individual: M31, galaxies: star clusters.
- Teeft :
- Absolute magnitude, Aperture photometry, Arcsec, Bekki chiba, Bergh, Bergh mackey, Bright stars, Brodie larsen, Cluster, Dsphs, Dwarf, Dwarf galaxy, Dwarf spheroidals, Galaxy, Giant galaxy, Globular clusters, Halo, Hilker infante, Host galaxies, Intermediate forms, Iraf implementation, Irwin, Irwin hatzidimitriou, Irwin lewis, Isaac newton telescope, Large number, Large radii, Larsen, Lenticular galaxies, Lled points, Luminosity, Luminous star clusters, Mnras, Parameter space, Photometry, Progenitor dwarf, Star cluster, Star clusters, Such clusters, Super star clusters, Tidal radii.
Abstract
We present three new clusters discovered in the halo of M31 which, although having globular‐like colours and luminosities, have unusually large half‐light radii, ∼30 pc. They lie at projected galactocentric distances of ≈15 to ≈35 kpc. These objects begin to fill the gap in parameter space between globular clusters and dwarf spheroidals, and are unlike any clusters found in the Milky Way, or elsewhere to date. Colour–magnitude diagrams, integrated photometric properties and derived King profile fit parameters are given, and we discuss possible origins of these clusters and their relationships to other populations.
Url:
- https://api.istex.fr/document/0C870C03071CCE64168D3CD2DAA11377352927EE/fulltext/pdf
- https://api.istex.fr/document/4E8B31D3D0BD5D3389DEB2DA101AB3BC35C69855/fulltext/pdf
DOI: 10.1111/j.1365-2966.2005.09086.x
Affiliations:
- Australie, Canada, France, Royaume-Uni
- Alsace (région administrative), Grand Est, Nouvelle-Galles du Sud, Écosse
- Strasbourg, Sydney, Édimbourg
- Université d'Édimbourg, Université de Sydney
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Le document en format XML
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<front><div type="abstract" xml:lang="en">We present three new clusters discovered in the halo of M31 which, although having globular‐like colours and luminosities, have unusually large half‐light radii, ∼30 pc. They lie at projected galactocentric distances of ≈15 to ≈35 kpc. These objects begin to fill the gap in parameter space between globular clusters and dwarf spheroidals, and are unlike any clusters found in the Milky Way, or elsewhere to date. Colour–magnitude diagrams, integrated photometric properties and derived King profile fit parameters are given, and we discuss possible origins of these clusters and their relationships to other populations.</div>
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