High velocity gas components associated with supergiant stars and interstellar gas

Details High velocity gas components associated with supergiant stars and interstellar gas High velocity gas components associated with supergiant stars and interstellar gas

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982esasp.176..403b&link_type=abstract

In ESA 3rd European IUE Conf. p 403-409 (SEE N83-11889 02-88)

Computer Science

7

Gas Composition, Interstellar Chemistry, Interstellar Gas, Supergiant Stars, Abundance, Electron Density (Concentration), Interstellar Extinction, Red Shift, Resonance Lines, Stellar Mass Ejection, Thematic Mapping, Ultraviolet Spectra

Scientific paper

Ultraviolet spectral data on the variability of expanding shells, associated with mass loss from Beta Ori, are presented. Red shifted high velocity gas components (HVC) observed in the interstellar gas in the line of sight towards HD 212593 (4 Lac) are discussed. A partial mapping of this material was obtained. Data suggest that HVC velocity = 80 km/sec, n (H) = 100 to 300 per cu cm, electron density 1/cu cm, and temperature = 1000 to 10,000 K. The strongest HVC feature may be associated with the intersection of galactic radio loops 1, 2, and 3.

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