Post SM4 HST Imaging Of The High Metallicity LGRB 051022 Host

Details Post SM4 HST Imaging Of The High Metallicity LGRB 051022 Host Post SM4 HST Imaging Of The High Metallicity LGRB 051022 Host

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21540511g&link_type=abstract

American Astronomical Society, AAS Meeting #215, #405.11; Bulletin of the American Astronomical Society, Vol. 42, p.229

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Scientific paper

We present our measurement of the dark LGRB 051022 host's metallicity at log(O/H)+12 = 8.77 (Kobulnicky & Kewley 2004 scale) the highest by a wide margin of any LGRB host, the luminosity metallicity redshift relation of this host to other LGRB hosts, Ic Supernovae hosts, and the general galaxy population, and our post SM4 HST imaging of the host galaxy in concert with astrometric alignment of the Chandra X-ray afterglow position, providing likely explanation for the host's high metal abundance and deviation from the typical LGRB host metal aversion.

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