Possible Alternative Counterparts to the SGR-like Event towards the Gamma-Ray Binary LS I+61 303

Details Possible Alternative Counterparts to the SGR-like Event towards the Gamma-Ray Binary LS I+61 303 Possible Alternative Counterparts to the SGR-like Event towards the Gamma-Ray Binary LS I+61 303

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..422..202m&link_type=abstract

High Energy Phenomena in Massive Stars ASP Conference Series, Vol. 422, proceedings of a conference held 2-5 February 2009 in Ja

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Scientific paper

We present an overview of a deep radio imaging of the LS I+61 303 field based on a combined analysis of archival data obtained with the Very Large Array (VLA) at the 6 cm wavelength. In addition to this well known gamma-ray binary, we find several radio sources inside the error box of the Soft Gamma-Ray Repeater (SGR) event recently observed towards it by the Swift satellite. None of them appears to display any special peculiarity which could indicate a different origin for the Swift flaring event other than LS I+61 303.

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