Possible and Suggested Historical Supernovae in the Galaxy
Various temporary stars recorded in history prior to the advent of the telescopic era have been proposed as possible supernovae in our Galaxy. Five of these stars – those first seen in the years AD 1006, 1054, 1181, 1572 and 1604 – remained visible for at least 6 months. These were recorded in detail in a variety of historical sources. All are well-established supernovae and their remnants have been confidently identified. Many further new stars have been recorded in East Asian history, some of which – ranging in date from the fourteenth century BC to AD 1592 – have been proposed as other possible sightings of supernovae. However, in most instances only a single brief record is extant, sometimes without any indication of the duration of visibility or a clear description of the celestial location. Here we consider these additional sightings, including those that have been suggested as supernovae.
KeywordsHistorical Record Supernova Remnant Ming Dynasty Galactic Latitude Official History
- B¨orner G, Qibin L, Aschenbach B (2001) Some possible identifications of ROSAT sources with historical SN events. In: Banday AJ, Zaroubi S, Bartelmann M (eds) Mining the sky. Springer, Heidelberg/New York, pp 649–655Google Scholar
- Chu SI (1973) Cas A as a supernova remnant (the supernova of the 16th century). J Korean Astron Soc 6:1–8Google Scholar
- Clark DH, Stephenson FR (1977) The historical supernovae. Pergamon Press, OxfordGoogle Scholar
- Green DA (2014) A catalogue of 294 Galactic supernova remnants. Bull Astron Soc India 42:47–58. See also http://www.mrao.cam.ac.uk/surveys/snrs/. Accessed 1 Nov 2015.
- Wang ZR (2001) A historical hypernova and the youngest pulsar. In: Inoue H, Kunieda H (eds) New century of X-ray astronomy. ASP conference proceedings, vol 251. Astronomical Society of the Pacific, San Francisco, pp 284–285Google Scholar