Extinction properties of the X-ray bright/optically faint afterglow of GRB 020405
arXiv:astro-ph/0506411 · doi:10.1051/0004-6361:20053302
Abstract
We present an optical-to-X-ray spectral analysis of the afterglow of GRB 020405. The optical spectral energy distribution not corrected for the extragalactic extinction is significantly below the X-ray extrapolation of the single powerlaw spectral model suggested by multiwavelength studies. We investigate whether considerable extinction could explain the observed spectral ``mismatch'' by testing several types of extinction curves. For the first time we test extinction curves computed with time-dependent numerical simulations of dust grains destruction by the burst radiation. We find that an extinction law weakly depen dent on wavelength can reconcile the unabsorbed optical and X-ray data with the expected synchrotron spectrum. A gray extinction law can be provided by a dust grain size distribution biased toward large grains.
arXiv comment6 pages, 5 figures, accepted for publication on A&A
References in corpus (34)
- Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
- Spectra and Light Curves of Gamma-Ray Burst Afterglows
- Discovery of the peculiar supernova 1998bw in the error box of GRB980425
- Spectroscopic Discovery of the Supernova 2003dh Associated with GRB 030329
- The Shape of Spectral Breaks in GRB Afterglows
- On The Synchrotron Self-Compton Emission from Relativistic Shocks and Its Implications for Gamma-Ray Burst Afterglows
- Reddening and Star Formation in Starburst Galaxies
- SN 2003lw and GRB 031203: A Bright Supernova for a Faint Gamma-ray Burst
- Dust sublimation by GRBs and its implications
- A supernova origin for dust in a high-redshift quasar
- High column densities and low extinctions of gamma-ray bursts: Evidence for hypernovae and dust destruction
- Dust in active nuclei. II. Powder or gravel?
- The host of GRB 030323 at z=3.372: a very high column density DLA system with a low metallicity
- Evidence for Supernova Signatures in the Spectrum of the Late-time Bump of the Optical Afterglow of GRB 021211
- X-ray Destruction of Dust Along the Line of Sight to Gamma-Ray Bursts
- Heavy Element Abundances and Dust Depletions in the Host Galaxies of Three Gamma-Ray Bursts
- Absorption in Gamma Ray Burst afterglows
- Very high column density and small reddening towards GRB 020124 at z = 3.20
- Time-Dependent Photoionization in a Dusty Medium II: Evolution of Dust Distributions and Optical Opacities
- Gamma-Ray Burst in a Molecular Cloud: Destruction of Dust and H2, and Emergent Spectrum
- Dust Depletion and Extinction in a Gamma-Ray Burst Afterglow
- Time-Dependent Photoionization in a Dusty Medium I: Code Description and General Results
- Optical and near-infrared observations of the GRB020405 afterglow
- Discovery of GRB 020405 and its Late Red Bump
- The Discovery and Broad-band Follow-up of the Transient Afterglow of GRB 980703
- A comparative study of the X-ray afterglow properties of optically bright and dark GRBs
- The Strongly Polarized Afterglow of GRB 020405
- GRB010222: afterglow emission from a rapidly decelerating shock
- The Broadband Afterglow of GRB980329
- A Radio Flare from GRB 020405: Evidence for a Uniform Medium Around a Massive Stellar Progenitor
- Colors and luminosities of the optical afterglows of the gamma-ray bursts
- Polarization Evolution of the GRB 020405 Afterglow
- High Resolution Grating Spectroscopy of GRB 020405 with CHANDRA LETGS
- The supernova associated with GRB 020405
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- Gamma-Ray Burst afterglows as probes of environment and blastwave physics I: absorption by host galaxy gas and dust
- Evidence for Supernova-Synthesised Dust from the Rising Afterglow of GRB 071025 at z~5
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- When Do Internal Shocks End and External Shocks Begin? Early-Time Broadband Modelling of GRB 051111
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- Determining the Dust Extinction of Gamma-ray Burst Host Galaxies: A Direct Method Based on Optical and X-ray Photometry
- An infrared ring around the magnetar SGR 1900+14
- A Direct Measurement of the Dust Extinction Curve in an Intermediate-Redshift Galaxy
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- Grey Milky Way Extinction from SDSS Stellar Photometry
- Probing the ambient medium of GRB 090618 with XMM-Newton observations
- Optical afterglows of gamma-ray bursts: a bimodal distribution?"
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