Multi-wavelength sources in the vicinity of LS I +61 303

Details Multi-wavelength sources in the vicinity of LS I +61 303 Multi-wavelength sources in the vicinity of LS I +61 303

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1740....1m&link_type=abstract

The Astronomer's Telegram, #1740

Astronomy and Astrophysics

Astronomy

9

Radio, Infra-Red, X-Ray, Gamma Ray, Binaries, Pulsars, Soft Gamma- Ray Repeaters, Transients

Scientific paper

Recently, a SGR-like burst was detected by the Swift BAT on 2008 September 10th (de Pasquale et al. GCN 8209). The BAT on-board location of the burst was placed at 140 arcsec from LS I +61 303 with a 3 arcmin location error. The ground calculated location was refined to an error of 2.2 arcmin placed at 88 arcsec from the High Mass X-ray Binary (Barthelmy et al. GCN 8215). It has been proposed that this burst has been associated to magnetar- like activity linked to the presence of a young highly magnetized pulsar in the binary system (Dubus & Giebels, Atel #1715).

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