GRB 090426-an oddball event in the outskirts of two interacting galaxies

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Gamma-Ray Sources (Astronomical), Redshift, Galaxies, Brightness, Gamma-Ray Sources, Gamma-Ray Bursts, Distances, Redshifts, Radial Velocities, Spatial Distribution Of Galaxies, Galaxy Clusters, Magnitudes And Colors, Luminosities

Scientific paper

GRB 090426 at a redshift of z = 2.609 had been classified as a ``short'' but with an exceptionally soft spectrum, placing it outside the normal short and long populations in the T90 vs. HR plot. It was the first short burst where an optical spectrum had been obtained. In contrast to other GRB afterglow spectra it shows exceptional properties indicating an almost fully ionized medium. The host galaxy is a complex of two large star-forming galaxies that are likely in the process of merging. Photoionization modeling of the metal column densities gives a distance of the absorbing material to the GRB of only 80pc, closer to what has been usually derived for the predominantly neutral material in other GRB spectra. The GRB thus likely exploded in an isolated star-forming region possibly created by the tidal interaction of the two galaxies.

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