The Scorpio-Centaurus Association: IV. Interstellar Absorption Lines in the Southern Milky Way

Abstract
From measures of the sharp K line in the spectra of 60 O and early B-type stars, radial velocities are derived for interstellar calcium clouds, mainly within a few hundred parsecs of the Sun. In directions where these clouds apparently coincide with neutral hydrogen at the same distance, there is close agreement between optical and radio velocities.

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