A radial velocity survey of low Galactic latitude structures – III. The Monoceros Ring in front of the Carina and Andromeda galaxies
Identifieur interne : 009A55 ( Main/Exploration ); précédent : 009A54; suivant : 009A56A radial velocity survey of low Galactic latitude structures – III. The Monoceros Ring in front of the Carina and Andromeda galaxies
Auteurs : N. F. Martin [France] ; M. J. Irwin ; R. A. Ibata [France] ; B. C. Conn [Australie] ; G. F. Lewis [Australie] ; M. Bellazzini [Italie] ; S. Chapman [États-Unis] ; N. TanvirSource :
- Monthly Notices of the Royal Astronomical Society: Letters [ 1745-3925 ] ; 2006-03.
English descriptors
- KwdEn :
- 2mass catalogue, Andromeda galaxy, Anticentre direction, Canis, Carina, Carina dwarf, Carina dwarf galaxy, Direct comparison, Disc, Disc population, Disc stars, Dispersion, Dwarf, Dwarf galaxy, Flames observations, Foreground, Galactic, Galactic components, Galactic disc, Galactic latitude structures, Galactic longitude, Galactic plane, Galactocentric distance, Galaxy, Galaxy: formation, Galaxy: structure, Gaussian model, Halo, Halo population, Halo stars, Hollow circles, Ibata, Irwin, Journal compilation, Lled circles, Main sequence, Mnras, Monoceros ring, Populations show, Previous detections, Primary targets, Radial, Radial velocities, Radial velocity, Radial velocity distribution, Radial velocity survey, Radial velocity values, Ring detection, Ring selection, Ring stars, Ring structure, Rotational velocity, Stellar halo, Thick disc, Velocity dispersion, Velocity distribution, galaxies: interactions.
- Teeft :
- 2mass catalogue, Andromeda galaxy, Anticentre direction, Canis, Carina, Carina dwarf, Carina dwarf galaxy, Direct comparison, Disc, Disc population, Disc stars, Dispersion, Dwarf, Dwarf galaxy, Flames observations, Foreground, Galactic, Galactic components, Galactic disc, Galactic latitude structures, Galactic longitude, Galactic plane, Galactocentric distance, Galaxy, Gaussian model, Halo, Halo population, Halo stars, Hollow circles, Ibata, Irwin, Journal compilation, Lled circles, Main sequence, Mnras, Monoceros ring, Populations show, Previous detections, Primary targets, Radial, Radial velocities, Radial velocity, Radial velocity distribution, Radial velocity survey, Radial velocity values, Ring detection, Ring selection, Ring stars, Ring structure, Rotational velocity, Stellar halo, Thick disc, Velocity dispersion, Velocity distribution.
Abstract
As part of our radial velocity survey of low Galactic latitude structures that surround the Galactic disc, we report the detection of the so‐called Monoceros Ring in the foreground of the Carina dwarf galaxy at Galactic coordinates (l, b) = (260°, −22°) based on Very Large Telescope/Fibre Large Array Multi Element Spectrograph observations of the dwarf galaxy. At this location, 20° in longitude greater than previous detections, the Ring has a mean radial velocity of 145 ± 5 km s−1 and a velocity dispersion of only 17 ± 5 km s−1. Based on Keck/Deep Imaging Multi‐Object Spectrograph observations, we also determine that the Ring has a mean radial velocity of −75 ± 4 km s−1 in the foreground of the Andromeda galaxy at (l, b) ∼ (122°, −22°), along with a velocity dispersion of 26 ± 3 km s−1. These two kinematic detections are both highly compatible with known characteristics of the structure and, along with previous detections, provide radial velocity values of the Ring over the 120° < l < 260° range. This should place strong constraints on numerical models of the accretion of the dwarf galaxy that is believed to be the progenitor of the Ring.
Url:
- https://api.istex.fr/document/A0D6E0608F845D52CE724D70B1AB938463E1304A/fulltext/pdf
- https://api.istex.fr/document/471DE312475110B4D63926802E0C75933E1BFB91/fulltext/pdf
DOI: 10.1111/j.1745-3933.2006.00142.x
Affiliations:
- Australie, France, Italie, États-Unis
- Alsace (région administrative), Grand Est, Nouvelle-Galles du Sud
- Strasbourg, Sydney
- Université de Sydney
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Le document en format XML
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<front><div type="abstract" xml:lang="en">As part of our radial velocity survey of low Galactic latitude structures that surround the Galactic disc, we report the detection of the so‐called Monoceros Ring in the foreground of the Carina dwarf galaxy at Galactic coordinates (l, b) = (260°, −22°) based on Very Large Telescope/Fibre Large Array Multi Element Spectrograph observations of the dwarf galaxy. At this location, 20° in longitude greater than previous detections, the Ring has a mean radial velocity of 145 ± 5 km s−1 and a velocity dispersion of only 17 ± 5 km s−1. Based on Keck/Deep Imaging Multi‐Object Spectrograph observations, we also determine that the Ring has a mean radial velocity of −75 ± 4 km s−1 in the foreground of the Andromeda galaxy at (l, b) ∼ (122°, −22°), along with a velocity dispersion of 26 ± 3 km s−1. These two kinematic detections are both highly compatible with known characteristics of the structure and, along with previous detections, provide radial velocity values of the Ring over the 120° < l < 260° range. This should place strong constraints on numerical models of the accretion of the dwarf galaxy that is believed to be the progenitor of the Ring.</div>
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