MSH 10-53 - A supernova remnant interacting with molecular clouds

Details MSH 10-53 - A supernova remnant interacting with molecular clouds MSH 10-53 - A supernova remnant interacting with molecular clouds

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...309..667r&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 309, Oct. 15, 1986, p. 667-673. Research supported by Universidad de Chile.

Astronomy and Astrophysics

Astronomy

15

Molecular Clouds, Supernova Remnants, Carbon Monoxide, Line Spectra, Radio Astronomy, Spectrophotometry, Spectrum Analysis

Scientific paper

Optical spectrophotometry and CO radio observations are presented that indicate the presence of a shock expanding and interacting with the surrounding molecular clouds. It is established that the shock originated in a supernova explosion (probably of a massive star) occurred some 10,000 yr ago at about 2.9 kpc from us in the near side of the Carina spiral arm.

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