The interaction of the supernova remnant VRO 42.05.01 with its H I environment

Details The interaction of the supernova remnant VRO 42.05.01 with its H I environment The interaction of the supernova remnant VRO 42.05.01 with its H I environment

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.237..277l&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 237, March 15, 1989, p. 277-297. Research supported by

Astronomy and Astrophysics

Astronomy

26

H I Regions, Interstellar Matter, Supernova Remnants, Ablation, Continuous Spectra, Mass Distribution, Molecular Clouds

Scientific paper

Observations of the SNR VRO 42.05.01 obtained with a resolution of 2 km/s in velocity and 4 arcmin in angle reveal the interaction of the SNR with the surrounding H I environment. The results support a model in which a blast wave has broken into and reenergized a prexisting low-density hot cavity after an initial expansion in a warm medium with a density of about 1/cu cm. The systemic velocity of the H I associated with the SNR is found to be -34 + or - 5 km/s.

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