Millimeter observations of the candidate soft gamma-ray repeater SGR 1814-13
Identifieur interne : 00CE83 ( Main/Merge ); précédent : 00CE82; suivant : 00CE84Millimeter observations of the candidate soft gamma-ray repeater SGR 1814-13
Auteurs : Ph. Durouchoux [France] ; R. Sood [Australie] ; I. Smith [États-Unis] ; S. Corbel [France] ; D. Hannikainen [Finlande] ; R. Loyer [France]Source :
- Advances in Space Research [ 0273-1177 ] ; 2000.
English descriptors
- KwdEn :
- Astrophys, Corbel, Durouchoux, Elsevier science, Galactic, Galactic rotation curve, Hurley, Hydrogen column density, Interstellar extinction, June, Kinematic distances, Kouveliotou, Millimeter observations, Molecular cloud, Mopra millimeter radio telescope, Private communication, Repeater, Second date, September, Sgrs, Soft repeater, Visual absorption.
- Teeft :
- Astrophys, Corbel, Durouchoux, Elsevier science, Galactic, Galactic rotation curve, Hurley, Hydrogen column density, Interstellar extinction, June, Kinematic distances, Kouveliotou, Millimeter observations, Molecular cloud, Mopra millimeter radio telescope, Private communication, Repeater, Second date, September, Sgrs, Soft repeater, Visual absorption.
Abstract
Abstract: A possible new soft Gamma-Ray Repeater, SGR 1814-13, was first detected on 1997 June 29, with a subsequent possible detection on 1997 September 12. We observed this region on 1997 October 28 and 29, with the MOPRA millimeter radio telescope, in the transition CO(1-0) at 115 GHz, and found a molecular cloud in the direction of this source. Assuming that this cloud is associated with SGR 1814-13, we have derived, from the Galactic rotation curve, kinematic distances of 1.3 kpc and 15 kpc to the source. From the CO (1-0) spectrum, we estimate a hydrogen column density of N(H2) = 5 × 1021 cm−2, and a visual absorption of Av = 5.7 mag. We present arguments for the source to be located at 15 kpc.
Url:
DOI: 10.1016/S0273-1177(99)00837-6
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<front><div type="abstract" xml:lang="en">Abstract: A possible new soft Gamma-Ray Repeater, SGR 1814-13, was first detected on 1997 June 29, with a subsequent possible detection on 1997 September 12. We observed this region on 1997 October 28 and 29, with the MOPRA millimeter radio telescope, in the transition CO(1-0) at 115 GHz, and found a molecular cloud in the direction of this source. Assuming that this cloud is associated with SGR 1814-13, we have derived, from the Galactic rotation curve, kinematic distances of 1.3 kpc and 15 kpc to the source. From the CO (1-0) spectrum, we estimate a hydrogen column density of N(H2) = 5 × 1021 cm−2, and a visual absorption of Av = 5.7 mag. We present arguments for the source to be located at 15 kpc.</div>
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