The Schweizer-Middleditch star - Not a stellar remnant of SN 1006

Details The Schweizer-Middleditch star - Not a stellar remnant of SN 1006 The Schweizer-Middleditch star - Not a stellar remnant of SN 1006

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...107l...3s&link_type=abstract

Astronomy and Astrophysics, vol. 107, no. 1, Mar. 1982, p. L3, L4.

Astronomy and Astrophysics

Astrophysics

7

Blue Stars, Stellar Evolution, Stellar Temperature, Supernova Remnants, White Dwarf Stars, Cosmology, Radiant Cooling, Stellar Spectrophotometry, Supernovae

Scientific paper

The blue star found by Schweizer and Middleditch (1980) near the center of SN1006 cannot be a stellar remnant of that supernova, unless it is considerably more exotic than is justified by existing observational data. Conventional stellar evolution theory shows that the time to cool to the observed effective temperature is approximately one million years, far in excess of the 975 year age of the supernova remnant.

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