Copernicus observations of interstellar matter toward 15 Monocerotis

Details Copernicus observations of interstellar matter toward 15 Monocerotis Copernicus observations of interstellar matter toward 15 Monocerotis

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...238..560s&link_type=abstract

Astrophysical Journal, Part 1, vol. 238, June 1, 1980, p. 560-564.

Other

10

Abundance, Interstellar Matter, Line Spectra, Ultraviolet Spectra, Molecular Gases, Nebulae, Oao 3, Spectral Line Width, Stellar Magnitude

Scientific paper

Copernicus ultraviolet data on interstellar lines towards 15 Monocerotis are analyzed to provide abundances, velocities, and physical conditions in both low- and intermediate-velocity components. This line of sight lies 5 deg from the center of the Monoceros Loop and is unusual in containing a positive intermediate-velocity absorption component, as well as a high-velocity feature in O VI. Silicon, and presumably other refractory elements, are nearly undepleted in this intermediate velocity feature, which may be related to the O VI.

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