Physics of our days

Supernova explosions and historical chronology

Russian Federation State Scientific Center A.I. Alikhanov Institute ofTheoretical and Experimental Physics, ul. Bolshaya Cheremushkinskaya 25, Moscow, 117259, Russian Federation

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.

PACS: 01.75.+m, 01.90.+g, 97.60.Bw, 98.58.Mj (all)
DOI: 10.1070/PU2000v043n05ABEH000753
Citation: Imshennik V S "Supernova explosions and historical chronology" Phys. Usp. 43 509–513 (2000)
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:    «   » 170 553–558 (2000); DOI: 10.3367/UFNr.0170.200005e.0553

References (11) ↓ Cited by (2) Similar articles (7)

  1. Nosovskiî G, Fomenko A Vvedenie v Novuyu Khronologiyu: Kakoî Seîchas Vek? (Introduction to a New Chronology: Which Century is it Now?, Moscow: Kraft+, Lean, 1999)
  2. Efremov Yu N, Zavenyagin Yu A "On the so called ’new chronology’ of A T Fomenko" Vestnik Ross. Akad. Nauk 69 1081 (1999)
  3. Supernovae and Supernova Remnants (IAU Colloquium, 145, Eds R McCray, Zh Wang, Cambridge: Cambridge Univ. Press, 1996)
  4. Shklovskiî I S Zvezdy: Ikh Rozhdenie, Zhizn’ i Smert’ (Stars: Their Birth, Life, and Death) 3nd ed. (Moscow: Nauka, 1984) [see also: Translated into English (San Francisco: W.H. Freeman, 1978)]
  5. Lozinskaya T A Sverkhnovye Zvezdy i Zvezdnyî Veter. Vzaimodeîstvie s Gazom Galaktiki (Supernovae and Stellar Wind. Interaction With Galactic Gas (Moscow: Nauka, 1986) [Translated into English: Supernovae and Stellar Wind in the Interstellar Medium (New York: American Institute of Physics, 1992)]
  6. Wang Zh "Historical Supernovae and Supernova Remnants", in Supernovae and Supernova Remnants (IAU Colloquium, 145, Eds R McCray, Zh Wang, Cambridge: Cambridge Univ. Press, 1996) p. 323
  7. Sedov L I Metody Podobiya i Razmernosti v Mekhanike (Similarity and Dimension Methods in Mechanics) 2nd ed. (M.-L: Gostekhizdat, 1951) [Translated into English (New York: Academic Press, 1959)]
  8. D’yachenko V F, Imshennik V S, Paleîchik V V "On the problem of motion of the interstellar matter due to nova or supernova explosion" Astron. Zh. 46 739 (1969)
  9. Hughes J P "The extraordinarily rapid expansion of the X-ray remnant of Kepler’s Supernova (SN 1604)" Astrophys. J. 527 298 (1999)
  10. Imshennik V S, Nadyozhin D K "Supernova 1987A in the Large Magellanic Cloud: observations and theory" Usp. Fiz. Nauk 156 561 (1988) [Sov. Phys. Usp. 31 461 (1988)]; in Soviet Scientific Reviews (1988-1989, Ser. E, Astrophysics and Space Physics, Vol. 7, Chur: Harwood Acad. Publ., 1989)]
  11. Diacon L Istoriya (History, Ed. G G Litavrin, Moscow: Nauka, 1988) p. 90

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