AustralieFrV1, Main, Exploration, bibRecord, 005941

SLICING THE MONOCEROS OVERDENSITY WITH SUPRIME-CAM

Identifieur interne : 005941 ( Main/Exploration ); précédent : 005940; suivant : 005942

SLICING THE MONOCEROS OVERDENSITY WITH SUPRIME-CAM

Auteurs : Blair C. Conn [Allemagne] ; Noelia E. D. Noël [Allemagne, Suisse] ; Hans-Walter Rix [Allemagne] ; Richard R. Lane [Chili] ; Geraint F. Lewis [Australie] ; Mike J. Irwin [Royaume-Uni] ; Nicolas F. Martin [Allemagne, France] ; Rodrigo A. Ibata [France] ; Andrew Dolphin [États-Unis] ; Scott Chapman [Royaume-Uni]

Source :

The Astrophysical journal [ 0004-637X ] ; 2012.

RBID : Pascal:12-0325646

Descripteurs français

Pascal (Inist)
- Distribution densité, Métallicité, Voie lactée, Diagramme magnitude couleur, Distance héliocentrique, Etoile proche, Modèle, Modélisation, Galaxies disques, Structure galaxies.

English descriptors

KwdEn :
- Color-magnitude diagrams, Density distribution, Disk galaxies, Galaxy structure, Heliocentric distance, Metallicity, Milky Way, Modelling, Models, Nearby stars.

Abstract

We derive distance, density, and metallicity distribution of the stellar Monoceros Overdensity (MO) in the outer Milky Way, based on deep imaging with the Subaru Telescope. We applied color-magnitude diagram fitting techniques in three stripes at galactic longitudes, l ∼ 130°, 150°, 170°, and galactic latitudes, +15° ≤ b ≤ +25°. The MO appears as a wall of stars at a heliocentric distance of ∼10.1 ± 0.5 kpc across the observed longitude range with no distance change. The MO stars are more metal-rich ([Fe/H] ∼ -1.0) than the nearby stars at the same latitude. These data are used to test three different models for the origin of the MO: a perturbed disk model, which predicts a significant drop in density adjacent to the MO that is not seen; a basic flared disk model, which can give a good match to the density profile but the MO metallicity implies the disk is too metal-rich to source the MO stars; and a tidal stream model, which, from the literature, brackets the distances and densities we derive for the MO, suggesting that a model can be found that would fully fit the MO data. Further data and modeling will be required to confirm or rule out the MO feature as a stream or as a flaring of the disk.

Affiliations:

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Le document en format XML

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<front><div type="abstract" xml:lang="en">We derive distance, density, and metallicity distribution of the stellar Monoceros Overdensity (MO) in the outer Milky Way, based on deep imaging with the Subaru Telescope. We applied color-magnitude diagram fitting techniques in three stripes at galactic longitudes, l ∼ 130°, 150°, 170°, and galactic latitudes, +15° ≤ b ≤ +25°. The MO appears as a wall of stars at a heliocentric distance of ∼10.1 ± 0.5 kpc across the observed longitude range with no distance change. The MO stars are more metal-rich ([Fe/H] ∼ -1.0) than the nearby stars at the same latitude. These data are used to test three different models for the origin of the MO: a perturbed disk model, which predicts a significant drop in density adjacent to the MO that is not seen; a basic flared disk model, which can give a good match to the density profile but the MO metallicity implies the disk is too metal-rich to source the MO stars; and a tidal stream model, which, from the literature, brackets the distances and densities we derive for the MO, suggesting that a model can be found that would fully fit the MO data. Further data and modeling will be required to confirm or rule out the MO feature as a stream or as a flaring of the disk.</div>
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<name sortKey="Ibata, Rodrigo A" sort="Ibata, Rodrigo A" uniqKey="Ibata R" first="Rodrigo A." last="Ibata">Rodrigo A. Ibata</name>
</country>
<country name="États-Unis"><noRegion><name sortKey="Dolphin, Andrew" sort="Dolphin, Andrew" uniqKey="Dolphin A" first="Andrew" last="Dolphin">Andrew Dolphin</name>
</noRegion>
</country>
</tree>
</affiliations>
</record>

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{{Explor lien
   |wiki=    Wicri/Asie
   |area=    AustralieFrV1
   |flux=    Main
   |étape=   Exploration
   |type=    RBID
   |clé=     Pascal:12-0325646
   |texte=   SLICING THE MONOCEROS OVERDENSITY WITH SUPRIME-CAM
}}

This area was generated with Dilib version V0.6.33.
Data generation: Tue Dec 5 10:43:12 2017. Site generation: Tue Mar 5 14:07:20 2024

	Serveur d'exploration sur les relations entre la France et l'Australie
	Attention, ce site est en cours de développement ! Attention, site généré par des moyens informatiques à partir de corpus bruts. Les informations ne sont donc pas validées.

Serveur d'exploration sur les relations entre la France et l'Australie

SLICING THE MONOCEROS OVERDENSITY WITH SUPRIME-CAM

SLICING THE MONOCEROS OVERDENSITY WITH SUPRIME-CAM

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Descripteurs français

English descriptors

Abstract

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