The Sigma-D relation for shell-like supernova remnants

Details The Sigma-D relation for shell-like supernova remnants The Sigma-D relation for shell-like supernova remnants

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...295l..13h&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 295, Aug. 1, 1985, p. L13-L16.

Astronomy and Astrophysics

Astrophysics

41

Brightness, Diameters, Molecular Clouds, Supernova Remnants, Absorption Spectra, Calibrating, Magellanic Clouds

Scientific paper

A large fraction of galactic supernova remnants, including a dozen shell-like remnants, can be associated with large molecular clouds or cloud complexes with well-determined distances. The Σ-D relation for these shell-like remnants, derived using distances to the associated molecular clouds, shows substantially smaller scatter than previous relations and establishes a good distance scale for shell-like remnants from Type II events.

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