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Interstellar sodium and Galactic structure. A high-resolution survey

Published online by Cambridge University Press:  04 August 2017

E. Maurice ,
A. Ardeberg  and
H. Lindgren
E. Maurice
Affiliation:
European Southern Observatory - La Silla Casilla 16317 Correo 9 Santiago de Chile
A. Ardeberg
Affiliation:
European Southern Observatory - La Silla Casilla 16317 Correo 9 Santiago de Chile
H. Lindgren
Affiliation:
European Southern Observatory - La Silla Casilla 16317 Correo 9 Santiago de Chile

Extract

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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.

Type
PART II: COMPOSITION, STRUCTURE AND KINEMATICS
Information
Symposium - International Astronomical Union , Volume 106: The Milky Way Galaxy , 1985 , pp. 325 - 328
Copyright
Copyright © Reidel 1985 

References

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