Supernova of AD 1437

Details Supernova of AD 1437 Supernova of AD 1437

Nov 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969natur.224..891m&link_type=abstract

Nature, Volume 224, Issue 5222, pp. 891 (1969).

Computer Science

1

Scientific paper

KIANG1 refers to the identification of the radio source CTB 35 as a supernova remnant and suggests a possible association with the Chinese supernova record of AD 1437. The only suggestion that CTB 35 is a supernova remnant was made by Braes and Hovenier2, who, incorrectly interpreting the radio data, deduced that CTB 35 had a non-thermal spectrum. In fact it has been shown from continuum observations3 and H109α recombination line measurements4 that CTB 35 is a thermal complex well identified with emission nebulae in this direction. The suggestion that it is a supernova remnant is not justified.

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