The host galaxy of GRB031203: a new spectroscopic study
arXiv:0709.0198 · doi:10.1051/0004-6361:20077698
Abstract
The host galaxy of the long-duration gamma-ray burst (GRB) 031203 (HG031203) 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. We analyse HG031203 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. HG031203 is a metal poor, actively star forming galaxy (star formation rate of 12.9+/-2.2 {M_{sun} yr^-1) at z=0.1054. From the emission-line analysis we derive an intrinsic reddening E_{HG}(B-V)\approx 0.4. This parameter doesn't show a compelling evidence of evolution at a month time-scale. We find an interstellar medium temperature of 12500 K and an electronic density of N_{e}=160 cm^-3. After investigating for possible Wolf-Rayet emission features in our spectra, we consider dubious the classification of HG031203 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; HG031203 is a clear outlier, with its really low metallicity (12+\log{O/H}=8.12+/-0.04).
12 pages, 10 figures. Accepted by A&A
References in corpus (44)
- Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
- Star Formation in Galaxies Along the Hubble Sequence
- The Origin of the Mass--Metallicity Relation: Insights from 53,000 Star-Forming Galaxies in the SDSS
- Collapsars - Gamma-Ray Bursts and Explosions in "Failed Supernovae"
- Discovery of the peculiar supernova 1998bw in the error box of GRB980425
- Long gamma-ray bursts and core-collapse supernovae have different environments
- Theories of Gamma-Ray Bursts
- Metallicities of 0.3<z<1.0 Galaxies in the GOODS-North Field
- Gamma-Ray Bursts in the Swift Era
- Swift detects a remarkable gamma-ray burst, GRB 060614, that introduces a new classification scheme
- The Gemini Deep Deep Survey. VII. The Redshift Evolution of the Mass-Metallicity Relation
- No supernovae associated with two long-duration gamma ray bursts
- The Composition Gradient in M101 Revisited. II. Electron Temperatures and Implications for the Nebular Abundance Scale
- An enigmatic long-lasting gamma-ray burst not accompanied by a bright supernova
- Dust in active nuclei. I. Evidence for "anomalous" properties
- The gamma-ray burst GRB060614 requires a novel explosive process
- SN 2003lw and GRB 031203: A Bright Supernova for a Faint Gamma-ray Burst
- UV star-formation rates of GRB host galaxies
- Gamma-Ray Bursts and Type Ic Supernovae: SN 1998bw
- A Spectroscopic Study of a Large Sample of Wolf-Rayet Galaxies
- Early-Time Photometry and Spectroscopy of the Fast Evolving SN 2006AJ Associated with GRB 060218
- The Host Galaxy of GRB 031203: Implications of its low metallicity, low redshift, and starburst nature
- Stellar evolution with rotation XIII: Predicted GRB rates at various Z
- Models for the Type Ic Hypernova SN 2003lw associated with GRB 031203
- An apparently normal gamma-ray burst with an unusually low luminosity
- On the nature of nearby GRB/SN host galaxies
- Detection of Wolf-Rayet stars in host galaxies of Gamma-Ray Bursts (GRBs): are GRBs produced by runaway massive stars ejected from high stellar density regions ?
- The metallicity dependence of the long-duration GRB rate from host galaxy luminosities
- The KPNO International Spectroscopic Survey. I. Description of the Survey
- Identifying the Environment and Redshift of GRB Afterglows from the Time-Dependence of Their Absorption Spectra
- The GRB 030329 host: a blue low metallicity subluminous galaxy with intense star formation
- The nature of the dwarf starforming galaxy associated with GRB 060218 / SN2006aj
- The discovery of an evolving dust scattered X-ray halo around GRB 031203
- A new type of long gamma--ray burst
- The supernova 2003lw associated with X-ray flash 031203
- The J-band Light Curve of SN 2003lw, Associated with GRB 031203
- The LCO/Palomar 10,000 km/sec Cluster Survey. II. Constraints on Large-Scale Streaming
- The H alpha Luminosity Function of Morphologically Classified Galaxies in the Sloan Digital Sky Survey
- Discovery of a supernova associated with GRB 031203: SMARTS Optical-Infrared Lightcurves from 0.2 to 92 days
- Metal Abundances of KISS Galaxies. II. Nebular Abundances of Twelve Low-Luminosity Emission-Line Galaxies
- Identifying Gamma-Ray Burst Remnants in Nearby Galaxies
- The host galaxies of long-duration GRBs in a cosmological hierarchical scenario
- On the calibration of the COBE/IRAS dust emission reddening maps
- Massive star-formation rates of gamma-ray burst host galaxies: an unobscured view in X-rays
Cited by in corpus (28)
- Measured Metallicities at the Sites of Nearby Broad-Lined Type Ic Supernovae and Implications for the SN-GRB Connection
- The Afterglows of Swift-era Gamma-Ray Bursts. I. Comparing pre-Swift and Swift era Long/Soft (Type II) GRB Optical Afterglows
- A new population of ultra-long duration gamma-ray bursts
- A new method for estimating the bolometric properties of Ibc SNe
- The Host Galaxies of Gamma-Ray Bursts II: A Mass-Metallicity Relation for Long-Duration Gamma-Ray Burst Host Galaxies
- Relativistic supernovae have shorter-lived central engines or more extended progenitors: the case of SN\,2012ap
- The Host Galaxies of Gamma-Ray Bursts I: ISM Properties of Ten Nearby Long-Duration GRB Hosts
- XRF 100316D / SN 2010bh and the Nature of Gamma Ray Burst Supernovae
- IFU observations of the GRB 980425/SN 1998bw host galaxy: emission line ratios in GRB regions
- Evidence for Late-stage Eruptive Mass-loss in the Progenitor to SN2018gep, a Broad-lined Ic Supernova: Pre-explosion Emission and a Rapidly Rising Luminous Transient
- The properties of SN Ib/c locations
- The Wolf-Rayet features and mass-metallicity relation of long-duration gamma-ray burst host galaxies
- Outliers from the Mass--Metallicity Relation II: A Sample of Massive Metal-Poor Galaxies from SDSS
- Modeling The GRB Host Galaxy Mass Distribution: Are GRBs Unbiased Tracers of Star Formation?
- Core-collapse, superluminous, and gamma-ray burst supernova host galaxy populations at low redshift: the importance of dwarf and starbursting galaxies
- On the distribution of stellar masses in gamma-ray burst host galaxies
- Host Galaxies of Type Ic and Broad-lined Type Ic Supernovae from the Palomar Transient Factory: Implication for Jet Production
- Gamma-ray burst supernovae as standardizable candles
- The Host Galaxies of Long-Duration Gamma-Ray Bursts
- The luminous host galaxy, faint supernova and rapid afterglow rebrightening of GRB 100418A
- A nearby GRB host prototype for z~7 Lyman-break galaxies: Spitzer-IRS and X-shooter spectroscopy of the host galaxy of GRB031203
- Reconciling the GRB rate and star formation histories
- ALMA CO Observations of the Host Galaxies of Long-duration Gamma-ray Bursts. I: Molecular Gas Scaling Relations
- Herschel/PACS Observations of the Host Galaxy of GRB 031203
- A nearby GRB host galaxy: VLT/X-shooter observations of HG 031203
- Swift/UVOT: 18 Years of Long GRB Discoveries and Advances
- Shock fronts in the long GRB031203 host galaxy
- Rapid Response Mode observations of GRB 160203A: Looking for fine-structure line variability at z=3.52