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The Line of Sight of ϵ Canis Majoris: Depletion and Extent of the Local Cloud
Published online by Cambridge University Press: 12 April 2016
Abstract
With new high resolution UV spectra of ϵ CMa we show that the gas column density in this sight-line is less than 4 1017 cm−2, that the neutral gas density is less than 10−5 cm−3 after the first 3 parsecs, and that the Local Cloud seems to be almost undepleted and to extend to no more than 0.6 pc in this direction.
- Type
- Part IV Clouds, Ionized Gas, and Particles in the Local ISM
- Information
- International Astronomical Union Colloquium , Volume 166: The Local Bubble and Beyond , 1997 , pp. 161 - 164
- Copyright
- Copyright © Springer-Verlag 1998