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Burenin, V. V.

doi:10.1023/a:1017526624073

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Prompt Optical Afterglows1

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2003

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“…The most remarkable afterglow observed by many observatories was in GRB 030329 (see i.g. Rumjantsev et al, 2003;Burenin et al, 2003), where supernova was probably detected by the features of spectra (Stanek et al, 2003). Konus-Wind observations of GRB 030329 are given in Fig.…”

Section: Prompt Optical Afterglowsmentioning

confidence: 99%

Physical Limits of Different Models of Cosmic Gamma-Ray Bursts

Бисноватый-Коган¹

2003

Chin. J. Astron. Astrophys.

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The present common view about GRB origin is related to cosmology, what is based on statistical analysis, and on measurements of the redshifts in the GRB optical afterglows of long GRB. No correlation is found between redshifts, GRB spectrum, and total GRB fluence. Comparison of KONUS and BATSE data about statistics and hard X-ray lines is done, and some differences are noted. Hard gamma-ray afterglows, prompt optical spectra, hard X-ray lines measurements could be important for farther insight into GRB origin. Possible possible connection of short GRB with soft gamma repeaters is discussed.

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Section: Prompt Optical Afterglowsmentioning

confidence: 99%

Physical Limits of Different Models of Cosmic Gamma-Ray Bursts

Бисноватый-Коган¹

2003

Chin. J. Astron. Astrophys.

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Cited by 1 publication

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Physical Limits of Different Models of Cosmic Gamma-Ray Bursts

Physical Limits of Different Models of Cosmic Gamma-Ray Bursts

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