On high-velocity interstellar gas toward Delta SCO

Details On high-velocity interstellar gas toward Delta SCO On high-velocity interstellar gas toward Delta SCO

Jul 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mnras.176p..45h&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 176, July 1976, p. 45P, 46P.

Astronomy and Astrophysics

Astronomy

2

Absorption Spectra, D Lines, Interstellar Gas, Line Spectra, High Speed, Interstellar Radiation, Sodium

Scientific paper

Independent observations of the Na I D2 line toward Delta Sco are described which show that the two high-velocity absorption components reported by Hicks et al. (1975) are not of normal interstellar origin. A portion of the spectrum of Delta Sco near the D2 line is presented, and it is proposed that the two absorption components may have been of atmospheric origin, although their separation and relative intensities do not suggest any obvious counterparts within the observed telluric spectrum.

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