Neutral hydrogen in the vicinity of the supernova remnant G 357.7-0.1

Details Neutral hydrogen in the vicinity of the supernova remnant G 357.7-0.1 Neutral hydrogen in the vicinity of the supernova remnant G 357.7-0.1

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988azh....65.1097g&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 65, Sept.-Oct. 1988, p. 1097-1099. In Russian.

Astronomy and Astrophysics

Astronomy

1

Hydrogen Clouds, Neutral Gases, Stellar Envelopes, Supernova Remnants, H Lines, Spatial Distribution, Stellar Mass, Stellar Winds

Scientific paper

H I observations around SNR G 357.7-0.1 (MSH 17-39) were made. It is found that around this object there is an expanding H I shell with the diameter of 168 pc and H I mass about 1.5×104M_sun;. The most probable mechanism of formation of this shell is stellar wind outflow from the star during its evolution on the main sequence. Estimates of the stellar mass (55 M_sun;) and of the gas mass ejected during the supernova explosion (47 M_sun;) were made.

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