The host galaxy of GRB 031203 a new spectroscopic study

Margutti, R.R.MarguttiChincarini, G.G.ChincariniCovino, S.S.CovinoGiommi, PaoloPaoloGiommi2020-09-172020-09-172007-11-01https://hdl.handle.net/20.500.13025/750Astronomy and Astrophysics, Volume 474, Issue 3, November II 2007, pp.815-826Aims The host galaxy of the long-duration gamma-ray burst (GRB) 031203 (HG 031203) offers a precious opportunity to study in detail the environment of a nearby GRB. The aim is to better characterize this galaxy and analyse the possible evolution with time of the spectroscopic quantities we derive. Methods We analyse HG 031203 using a set of optical spectra acquired with the ESO-VLT and Keck telescope. We compare the metallicity, luminosity and star formation properties of this galaxy and of the other supernova-long gamma-ray burst hosts in the local universe (z < 0.2) against the KPNO International Spectroscopic Survey. Results HG 031203 is a metal poor, actively star forming galaxy (star formation rate of 12.92.2 M&sun; yr-1) at z = 0.1054. From the emission-line analysis we derive an intrinsic reddening EHG(B-V) ≈ 0.4. This parameter doesn't show a compelling evidence of evolution at a month time-scale. We find an interstellar medium temperature of ≈ 12 500 K and an electronic density of Ne = 160 cm-3. After investigating for possible Wolf-Rayet emission features in our spectra, we consider dubious the classification of HG 031203 as a Wolf-Rayet galaxy. Long gamma-ray burst (LGRB) and supernova hosts in the local universe (z < 0.2) show, on average, specific star formation rates higher than ordinary star forming galaxy at the same redshift. On the other hand, we find that half of the hosts follows the metallicity-luminosity relation found for star-burst galaxies; HG 031203 is a clear outlier, with its really low metallicity (12+log(O/H) = 8.120.04).gamma rays burstsgalaxies individual GRB 031203ISM abundancesstars Wolf-RayetThe host galaxy of GRB 031203 a new spectroscopic study10.1051/0004-6361 20077698http://adsabs.harvard.edu/abs/2007A&A...474..815M2007A&A...474..815M