[EGH2001b] B1 , the SIMBAD biblio

2005ApJ...623L.125K - Astrophys. J., 623, L125-L128 (2005/April-3)

A variable infrared counterpart to the soft gamma-ray repeater Sgr 1806-20.

KOSUGI G., OGASAWARA R. and TERADA H.

Abstract (from CDS):

We present K'-band (2.12 µm) imaging observations of the SGR 1806-20 field taken during its very active phase in mid-2004; these observations reveal brightening of sources within the Chandra X-ray error circle when compared with earlier images obtained in 2002. One source brightened by more than a factor of 2, and so we consider this to be the probable infrared counterpart to SGR 1806-20. The other two sources are located in close proximity to the probable counterpart and show marginal brightening, which may suggest that the high-energy photons emitted from the soft gamma-ray repeater (SGR) during its active phase have induced dust sublimation or brightening of the unresolved background around the SGR.

Abstract Copyright:

Journal keyword(s): Gamma Rays: Bursts - Stars: Pulsars: Individual: Alphanumeric: SGR 1806-20 - Stars: Neutron - X-Rays: Stars

Nomenclature: Fig.2, Table 1: [EGH2001b] AN (Nos A1-A4, B1-B3, F1-F7) added.

Simbad objects: 23

goto View the reference in ADS


2019.12.08-15:05:43

© Université de Strasbourg/CNRS

    • Contact