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Interstellar sodium and Galactic structure. A high-resolution survey

  • E. Maurice (a1), A. Ardeberg (a1) and H. Lindgren (a1)

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Observation of absorption lines produced by interstellar gas is a straight-forward way to determine column densities and velocities along the line of sight of interstellar clouds. In practice, peculiar motions often mask galactic rotation and/or cause line blending. We have made a study of absorption lines of interstellar sodium covering a substantial part of the Galaxy at extremely high spectral resolution.

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References

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Ardeberg, A., and Maurice, E.: 1980, Astron. Astrophys. Suppl. 39, 325
Ardeberg, A., and Maurice, E.: 1981, Astron. Astrophys. 98, 9
Georgelin, Y.P., and Georgelin, Y.M.: 1976, Astron. Astrophys. 49, 57
Rickard, J.J.: 1974, Astron. Astrophys. 31, 47
Schild, R., Neugebauer, G., and Westphal, J.A.: 1971, Astron. J. 76, 237
Schmidt, M.: 1965, in “Stars and Stellar Systems V”, Blaauw, A. and Schmidt, M. (eds.), 513

Interstellar sodium and Galactic structure. A high-resolution survey

  • E. Maurice (a1), A. Ardeberg (a1) and H. Lindgren (a1)

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