SIMBAD references

1999ApJ...526L..29C - Astrophys. J., 526, L29-L32 (1999/November-3)

The distance to the soft gamma repeater Sgr 1627-41.

CORBEL S., CHAPUIS C., DAME T.M. and DUROUCHOUX P.

Abstract (from CDS):

We report millimeter observations of the line of sight to the recently discovered soft gamma repeater SGR 1627-41, which has been tentatively associated with the supernova remnant (SNR) G337.0-0.1. Among the eight molecular clouds along the line of sight to SGR 1627-41, we show that SNR G337.0-0.1 is probably interacting with one of the most massive giant molecular clouds (GMCs) in the Galaxy, at a distance of 11 kpc from the Sun. Based on the high extinction to the persistent X-ray counterpart of SGR 1627-41, we present evidence for an association of this new soft gamma repeater (SGR) with the SNR G337.0-0.1; they both appear to be located on the near side of the GMC. This is the second SGR located near an extraordinarily massive GMC. We suggest that SGR 1627-41 is a neutron star with a high transverse velocity (∼1000 km.s–1) escaping the young (∼5000 yr) SNR G337.0-0.1.

Abstract Copyright:

Journal keyword(s): Gamma Rays: Bursts - ISM: individual (CTB 33, G337.0-0.1) - Stars: Individual: Alphanumeric: SGR 1627-41 - Stars: Neutron

Nomenclature: Table 1: [CCD99] MC -VVV N=8.

Simbad objects: 15

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:1999ApJ...526L..29C and select 'bookmark this link' or equivalent in the popup menu


2019.09.23-12:34:34

© Université de Strasbourg/CNRS

    • Contact