Specifying the environments around GRB, explaining the Fe line in the X-ray afterglow of GRB 000214

Publications of the Astronomical Society of Japan

Volumn 53, Issue 4, 2001, Pages 579-587

  Kotake, Kei ^a   Nagataki, Shigehiro ^a  

^a UNIVERSITY OF TOKYO   (Japan)

Author keywords

Gamma rays: Bursts; Gamma rays: Individual (GRB 000214); Ism: Supernova remnants; Line: Formation; X rays: General

Indexed keywords

ATOMS; COSMOLOGY; RELATIVITY; SUPERNOVAE;

CONTINUUM SPECTRUM; GAMMA RAYS BURSTS; GAMMA-RAY: INDIVIDUAL (GRB 000214); GAMMA-RAYS; ISM: SUPERNOVA REMNANTS; KΑ; LINE FORMATIONS; NATURAL ENVIRONMENTS; X-RAY AFTERGLOW; X-RAY GENERAL;

GAMMA RAYS;

EID: 0035539421     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/53.4.579     Document Type: Article

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