The interstellar medium near the sun - The line of sight to lambda Scorpii

Details The interstellar medium near the sun - The line of sight to lambda Scorpii The interstellar medium near the sun - The line of sight to lambda Scorpii

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...196l.103y&link_type=abstract

Astrophysical Journal, vol. 196, Mar. 15, 1975, pt. 2, p. L103-L106.

Astronomy and Astrophysics

Astronomy

77

Abundance, Interstellar Matter, Solar Position, H I Regions, H Ii Regions, Oao 3, Satellite Observation, Spaceborne Astronomy, Ultraviolet Spectra

Scientific paper

Copernicus satellite spectrometric observations are used to determine column densities and ionization structure in the local interstellar medium in the line of sight to lambda Sco. Three, or possibly four, regions are identified by physical properties or velocity separations in the UV absorption line profiles, including a region with a temperature near 200,000 K containing O VI lines, one or two H II regions, and an H I region which may also contain S III and C III. Element abundances are tabulated, and abundances in the H I region are shown to have a depletion pattern similar to that for the line of sight to zeta Oph.

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