Afterglow from GRB 070610/Swift J195509.6+261406: An explanation using the fireball model

Details Afterglow from GRB 070610/Swift J195509.6+261406: An explanation using the fireball model Afterglow from GRB 070610/Swift J195509.6+261406: An explanation using the fireball model

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010scchg..53s..94k&link_type=abstract

Science China Physics, Mechanics and Astronomy, Volume 53, Issue 1, pp.94-97

Astronomy and Astrophysics

Astronomy

Gamma-Ray Bursts, Soft Gamma-Ray Repeaters, Outflows

Scientific paper

GRB 070610, which is also named Swift J195509.6+261406, is a peculiar Galactic transient with significant variability on short timescales in both X-ray and optical light curves. One possible explanation is that GRB 070610/Swift J195509.6 + 261406 is a soft gamma-ray repeater (SGR) in our Galaxy. Here, we use the fireball model, which is usually recognized as the standard model of gamma-ray burst (GRB) afterglows, and the energy injection hypothesis to interpret the X-ray and optical afterglow light curves of GRB 070610/Swift J195509.6 + 261406. It is found that the model is generally consistent with observations.

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