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Uspekhi Fizicheskikh Nauk, 2000, Volume 170, Number 5, Pages 553–558
DOI: https://doi.org/10.3367/UFNr.0170.200005e.0553
(Mi ufn1758)
 

This article is cited in 2 scientific papers (total in 2 papers)

PHYSICS OF OUR DAYS

Supernova explosions and historical chronology

V. S. Imshennik

State Scientific Center of the Russian Federation - Institute for Theoretical and Experimental Physics, Moscow
References:
Abstract: Since ancient times (14th century BC), the so called 'new stars' and 'guest stars' — now known as supernova explosions, the strongest star explosions according to current views — have attracted the attention of man. The observed behavior of these stars was recorded most systematically in Chinese chronicles. In the present paper, age estimates for our galaxy's youngest (within the past millennium) supernova remnants are attempted using the simplest means of modern theoretical astrophysics. In most (five out of seven) cases such estimates are found to agree to within 100 years with their recorded dates, while in the two remaining cases a more elaborate analysis removes the significant differences obtained. The presence of pulsars in supernova remnants suggests alternative, independent approaches to supernova age estimation. The major conclusion is that the astrophysical determination of the age of the recorded supernova explosions confirms their historical chronology over the last 1200 years at least.
Received: March 10, 2000
English version:
Physics–Uspekhi, 2000, Volume 43, Issue 5, Pages 509–513
DOI: https://doi.org/10.1070/PU2000v043n05ABEH000753
Bibliographic databases:
Document Type: Article
PACS: 01.75.+m, 01.90.+g, 97.60.Bw, 98.58.Mj
Language: Russian


Citation: V. S. Imshennik, “Supernova explosions and historical chronology”, UFN, 170:5 (2000), 553–558; Phys. Usp., 43:5 (2000), 509–513
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  • This publication is cited in the following 2 articles:
    Citing articles in Google Scholar: Russian citations, English citations
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