Flux variability from the likely IR counterpart of SGR 1806-20

Details Flux variability from the likely IR counterpart of SGR 1806-20 Flux variability from the likely IR counterpart of SGR 1806-20

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..439....1i&link_type=abstract

The Astronomer's Telegram, #439

Astronomy and Astrophysics

Astronomy

1

Infra-Red, Soft Gamma-Ray Repeaters

Scientific paper

Following the refined radio position of SGR 1806-20 (Gaensler et al., astro-ph/0502393; Cameron et al., astro-ph/0502428), about 0.5" away from the preliminary one (Kouveliotou et al. 2005, GCN #2929), we note that the possible counterpart we tentatively identified (Israel et al., ATel #378) is not anymore included in the radio positional uncertainty region. Only one relatively faint object falls within the refined radio position regions, while two additional objects are just outside.

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