AustralieFrV1, Main, Exploration, bibRecord, 008811

Globular clusters in the outer halo of M31: the survey

Identifieur interne : 008811 ( Main/Exploration ); précédent : 008810; suivant : 008812

Globular clusters in the outer halo of M31: the survey

Auteurs : A. P. Huxor [Royaume-Uni] ; N. R. Tanvir ; A. M. N. Ferguson [Royaume-Uni] ; M. J. Irwin ; R. Ibata [France] ; T. Bridges [Canada] ; G. F. Lewis [Australie]

Source :

Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2008-04-21.

RBID : ISTEX:362C6E08D261F3B956AF56DB03074589E0C02846

Descripteurs français

Pascal (Inist)
- Amas galaxies, Amas globulaire, Amas stellaire, Catalogue astronomique, Evolution galaxies, Formation galaxies, Galaxies, Halo galaxies, Photométrie.

English descriptors

KwdEn :
- Arcsec, Arcsec aperture, Arcsec radius, Astronomical catalogues, Barmby, Barmby huchra, Basic properties, Bellazzini, Bologna catalogue, Bright star, Brodie strader, Calchi novati, Centre, Cluster, Colour, Diffuse cluster, Direct comparison, Dwarf galaxies, Federici, Fusi, Fusi pecci, Galactocentric distance, Galaxies, Galaxy, Galaxy clusters, Galaxy evolution, Galaxy formation, Galaxy halo, Galleti, Globular, Globular clusters, Halo, Huxor, Ibata, Image width, Inner ellipse, Irwin, Isaac newton camera, Joint project, Journal compilation, Limited extent, Line outlines, Many candidates, Mcconnachie, Megacam, Megacam survey, Mnras, National research council, Original bologna catalogue, Other regions, Outer halo, Parameter space, Pecci, Perrett, Photographic plates, Photometry, Previous surveys, Puzia, Spatial extent, Spectroscopic, Spiral galaxy, Star clusters, Stellar, Survey area, Tanvir, Target clusters, Visible disc.
Teeft :
- Arcsec, Arcsec aperture, Arcsec radius, Barmby, Barmby huchra, Basic properties, Bellazzini, Bologna catalogue, Bright star, Brodie strader, Calchi novati, Centre, Cluster, Colour, Diffuse cluster, Direct comparison, Dwarf galaxies, Federici, Fusi, Fusi pecci, Galactocentric distance, Galaxy, Galleti, Globular, Globular clusters, Halo, Huxor, Ibata, Image width, Inner ellipse, Irwin, Isaac newton camera, Joint project, Journal compilation, Limited extent, Line outlines, Many candidates, Mcconnachie, Megacam, Megacam survey, Mnras, National research council, Original bologna catalogue, Other regions, Outer halo, Parameter space, Pecci, Perrett, Photographic plates, Photometry, Previous surveys, Puzia, Spatial extent, Spectroscopic, Spiral galaxy, Star clusters, Stellar, Survey area, Tanvir, Target clusters, Visible disc.

Abstract

We report the discovery of 40 new globular clusters (GCs) that have been found in surveys of the halo of M31 based on the Isaac Newton Telescope/Wide‐Field Camera and Canada–France–Hawaii Telescope/Megacam imagery. A subset of these new GCs are of an extended, diffuse nature and include those already found in Huxor et al. The search strategy is described and basic positional and V and I photometric data are presented for each cluster. For a subset of these clusters, K‐band photometry is also given. The new clusters continue to be found to the limit of the survey area (∼100 kpc), revealing that the GC system of M31 is much more extended than previously realized. The new clusters increase the total number of confirmed GCs in M31 by approximately 10 per cent and the number of confirmed GCs beyond 1° (≈14 kpc) by more than 75 per cent. We have also used the survey imagery as well recent Hubble Space Telescope archival data to update the Revised Bologna Catalogue of M31 globular clusters.

Url:

DOI: 10.1111/j.1365-2966.2008.12882.x

Affiliations:

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<front><div type="abstract" xml:lang="en">We report the discovery of 40 new globular clusters (GCs) that have been found in surveys of the halo of M31 based on the Isaac Newton Telescope/Wide‐Field Camera and Canada–France–Hawaii Telescope/Megacam imagery. A subset of these new GCs are of an extended, diffuse nature and include those already found in Huxor et al. The search strategy is described and basic positional and V and I photometric data are presented for each cluster. For a subset of these clusters, K‐band photometry is also given. The new clusters continue to be found to the limit of the survey area (∼100 kpc), revealing that the GC system of M31 is much more extended than previously realized. The new clusters increase the total number of confirmed GCs in M31 by approximately 10 per cent and the number of confirmed GCs beyond 1° (≈14 kpc) by more than 75 per cent. We have also used the survey imagery as well recent Hubble Space Telescope archival data to update the Revised Bologna Catalogue of M31 globular clusters.</div>
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Globular clusters in the outer halo of M31: the survey

Globular clusters in the outer halo of M31: the survey

Source :

Descripteurs français

English descriptors

Abstract

Links toward previous steps (curation, corpus...)

Le document en format XML

Pour manipuler ce document sous Unix (Dilib)

Pour mettre un lien sur cette page dans le réseau Wicri

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