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Millimeter observations of the candidate soft gamma-ray repeater SGR 1814-13

Identifieur interne : 00BF70 ( Main/Exploration ); précédent : 00BF69; suivant : 00BF71

Millimeter 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 :

RBID : ISTEX:8E4DC373B5E56794AEC65355F04DE73E10B87B3E

English descriptors

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


Affiliations:


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Le document en format XML

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