High velocity gas associated with supernova remnants

Details High velocity gas associated with supernova remnants High velocity gas associated with supernova remnants

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980esasp.157..109g&link_type=abstract

The second European International Ultraviolet Explorer (IUE) Conference, held 26-28 March 1980 in Tübingen, West Germany. Edited

Astronomy and Astrophysics

Astronomy

2

Absorption Spectra, Interstellar Gas, Iue, Stellar Spectra, Supernovae, Ultraviolet Astronomy, Carbon Monoxide, Doppler Effect, Extraterrestrial Radiation, High Speed, Iron, Magnesium

Scientific paper

High dispersion International Ultraviolet Explorer spectra of early type background stars were obtained. An analysis was made of absorption lines originating in gas associated with the remnant S147 and the detection of gas associated with the remnant IC443. In the star HD 36665 behind S147, high velocity lines and low velocity interstellar CO was detected, probably originating in gas associated with the remnant.

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