A metal rich molecular cloud surrounds GRB 050904 at redshift 6.3
arXiv:astro-ph/0611305 · doi:10.1086/510719
Abstract
GRB050904 is the gamma-ray burst with the highest measured redshift. We performed time resolved X-ray spectroscopy of the late GRB and early afterglow emission. We find robust evidence for a decrease with time of the soft X-ray absorbing column. We model the evolution of the column density due to the flash ionization of the GRB and early afterglow photons. This allows us to constrain the metallicity and geometry of the absorbing cloud. We conclude that the progenitor of GRB050904 was a massive star embedded in a dense metal enriched molecular cloud with Z~0.03 Z_solar. This is the first local measurement of metallicity in the close environment of a GRB and one of the highest redshift metallicity measurements. We also find that the dust associated with the cloud cannot be similar to that of our Galaxy but must be either sizably depleted or dominated by silicate grains. We discuss the implications of these results for GRB progenitors and high redshift star formation.
arXiv comment4 pages, 2 figures. Accepted for publication on Astrophysical Journal Letters
References in corpus (28)
- Discovery of the peculiar supernova 1998bw in the error box of GRB980425
- A very energetic supernova associated with the gamma-ray burst of 29 March 2003
- Spectroscopic Discovery of the Supernova 2003dh Associated with GRB 030329
- The First Stars
- The shock break-out of GRB 060218/SN 2006aj
- Dust Formation in Primordial Type II Supernovae
- Bright X-ray Flares in Gamma-Ray Burst Afterglows
- SN 2003lw and GRB 031203: A Bright Supernova for a Faint Gamma-ray Burst
- Implications for the Cosmic Reionization from the Optical Afterglow Spectrum of the Gamma-Ray Burst 050904 at z = 6.3
- Dust sublimation by GRBs and its implications
- Molecular Gas in the Host Galaxy of a Quasar at Redshift z=6.42
- The Metallicity of High Redshift Galaxies: The Abundance of Zinc in 34 Damped Lyman Alpha Systems from z = 0.7 to 3.4
- The UCSD HIRES/KeckI Damped Lya Abundance Database: II. The Implications
- Massive-Star Supernovae as Major Dust Factories
- High-excitation CO in a quasar host galaxy at z=6.42
- The Giant X-ray Flare of GRB 050502B: Evidence for Late-Time Internal Engine Activity
- Dust Formation in Very Massive Primordial Supernovae
- Dissecting the Circumstellar Environment of Gamma-Ray Burst Progenitors
- Discovery and identification of the very high redshift afterglow of GRB 050904
- GRB 050904 at redshift 6.3: observations of the oldest cosmic explosion after the Big Bang
- VLT observations of the z=6.28 quasar SDSS 1030+0524
- Time-Dependent Photoionization in a Dusty Medium I: Code Description and General Results
- Detection of a very bright optical flare from a gamma-ray burst at redshift 6.29
- Identifying the Environment and Redshift of GRB Afterglows from the Time-Dependence of Their Absorption Spectra
- A flash in the dark: UVES/VLT high resolution spectroscopy of GRB afterglows
- Detection of a huge explosion in the early Universe
- An Energetic Afterglow From A Distant Stellar Explosion
- Outshining the quasars at reionisation: The X-ray spectrum and lightcurve of the redshift 6.29 Gamma-Ray Burst GRB050904
Cited by in corpus (48)
- Gamma-Ray Bursts in the Swift Era
- Star Formation History up to z = 7.4: Implications for Gamma-Ray Bursts and the Cosmic Metallicity Evolution
- Very different X-ray to optical column density ratios in gamma-ray burst afterglows: ionisation in GRB environments
- GRB 061121: Broadband spectral evolution through the prompt and afterglow phases of a bright burst
- The Galactic dust-to-metals ratio and metallicity using gamma-ray bursts
- X-ray Hardness Evolution in GRB Afterglows and Flares: Late Time GRB Activity Without N_H Variations
- GRB 100219A with X-shooter - abundances in a galaxy at z = 4.7
- The X-ray absorbing column densities of Swift Gamma-ray bursts
- The nature of GRB-selected submillimeter galaxies: hot and young
- A Survey for NV Absorption at z~z_GRB in GRB Afterglow Spectra: Clues to Gas Near the Progenitor Star
- The X-ray absorbing column density of a complete sample of bright Swift Gamma-Ray Bursts
- Dust properties at z=6.3 in the host galaxy of GRB 050904
- Gamma-Ray Burst afterglows as probes of environment and blastwave physics I: absorption by host galaxy gas and dust
- X-ray absorption evolution in Gamma-Ray Bursts: intergalactic medium or evolutionary signature of their host galaxies?
- Behavior of X-Ray Dust Scattering and Implications for X-Ray Afterglows of Gamma-Ray Bursts
- GRB 070306: A Highly Extinguished Afterglow
- A search for thermal X-ray signatures in Gamma-Ray Bursts I: Swift bursts with optical supernovae
- Detection of GRB 060927 at z = 5.47: Implications for the Use of Gamma-Ray Bursts as Probes of the End of the Dark Ages
- Variable Ly alpha sheds light on the environment surrounding GRB 090426
- Modelling the spectral response of the Swift-XRT CCD camera: Experience learnt from in-flight calibration
- Can the soft X-ray opacity towards high redshift sources probe the missing baryons?
- The properties of the host galaxy and the immediate environment of GRB 980425 / SN 1998bw from the multi-wavelength spectral energy distribution
- Helium in natal HII regions: the origin of the X-ray absorption in gamma-ray burst afterglows
- No evidence for dust extinction in GRB 050904 at z ~ 6.3
- An Evolving Stellar Initial Mass Function and the Gamma-Ray Burst Redshift Distribution
- Gamma Ray Bursts from the early Universe: predictions for present-day and future instruments
- Dust extinction bias in the column density distribution of gamma-ray bursts; high column density, low redshift GRBs are more heavily obscured
- Testing the Possible Intrinsic Origin of the Excess of Very Strong MgII Absorbers Along GRB Lines-of-Sight
- Is GRB 050904 at z=6.3 absorbed by dust?
- The dependence of gamma-ray burst X-ray column densities on the model for Galactic hydrogen
- The variable absorption in the X-ray spectrum of GRB 190114C
- A Direct Measurement of the Dust Extinction Curve in an Intermediate-Redshift Galaxy
- Constraining the Molecular Gas in the Environs of a z~8 Gamma Ray Burst Host Galaxy
- Gamma Ray Bursts as Probes of the Distant Universe
- Spectral Hardening Reveals Afterglow Emergence in Long-Duration Fast X-ray Transients: A Case Study of GRB 250404A/EP250404a
- Fires in the deep: The luminosity distribution of early-time gamma-ray-burst afterglows in light of the Gamow Explorer sensitivity requirements
- Searching for narrow absorption and emission lines in XMM-Newton spectra of gamma-ray bursts
- Investigating time variability of X-ray absorption in Swift GRBs
- Probing the ambient medium of GRB 090618 with XMM-Newton observations
- X-ray absorbing column densities of a complete sample of short Gamma Ray Bursts
- Evidence of Contribution of Intervening Clouds to GRB's X-ray Column Density
- Diverse Properties of Interstellar Medium Embedding Gamma-Ray Bursts at the Epoch of Reionization
- Examining the evidence for dust destruction in GRB 980703
- The metallicity of gamma-ray burst environments from high energy observations
- Probing the very high redshift Universe with Gamma-ray Bursts: prospects for observations with future X-ray instruments
- Rapid Response Mode observations of GRB 160203A: Looking for fine-structure line variability at z=3.52
- Exploration of the high-redshift universe enabled by THESEUS
- Time Evolution of Optical Darkness in GRB Afterglow: The Case of GRB 240825A