Iron line in the afterglow: a key to unveil gamma-ray burst progenitors
Open Access
- 7 April 1999
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 304 (2) , L31-L35
- https://doi.org/10.1046/j.1365-8711.1999.02517.x
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This publication has 21 references indexed in Scilit:
- Expected Characteristics of the Subclass of Supernova Gamma-Ray BurstsThe Astrophysical Journal, 1998
- On the Association of Gamma-Ray Bursts with SupernovaeThe Astrophysical Journal, 1998
- The edge of a gamma-ray burst afterglowMonthly Notices of the Royal Astronomical Society, 1998
- Spectral Features from Ultrarelativistic Ions in Gamma-Ray Bursts?The Astrophysical Journal, 1998
- Are Gamma-Ray Bursts in Star-Forming Regions?The Astrophysical Journal, 1998
- Spectral constraints on the redshift of the optical counterpart to the γ-ray burst of 8 May 1997Nature, 1997
- Supernova 1987A RevisitedAnnual Review of Astronomy and Astrophysics, 1993
- Nucleosynthesis, neutrino bursts and γ-rays from coalescing neutron starsNature, 1989
- Gamma-ray bursters at cosmological distancesThe Astrophysical Journal, 1986
- X-ray line spectroscopy for clusters of galaxies. IThe Astrophysical Journal, 1978