The distribution of novae and supernova remnants in the Large Magellanic Cloud

Details The distribution of novae and supernova remnants in the Large Magellanic Cloud The distribution of novae and supernova remnants in the Large Magellanic Cloud

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pasp..100.1486v&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 100, Dec. 1988, p. 1486-1488.

Astronomy and Astrophysics

Astronomy

8

Magellanic Clouds, Novae, Star Distribution, Supernova Remnants, Early Stars, Spatial Distribution

Scientific paper

Novae in the LMC appear to be distributed like an old disk population. The fact that no concentration of novae is seen within the Bar of the Large Cloud suggests that this feature is of relatively recent origin. Supernova remnants are seen to exhibit concentrations in the 30 Dor region, in the Bar of the Large Cloud, and in Constellation III. This distribution supports the idea that most of the supernova remnants in the LMC had young massive progenitors.

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