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III. Local Galactic Structure

Published online by Cambridge University Press:  25 April 2016

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This section contains work dealing with the Milky Way characteristics in the solar neighbourhood and supported by observations with wavelengths shorter than 1 mm. Thus, results are collected from gamma-ray, X-ray, UV, optical and IR observations in the different subsections. These are (1) the volume closest to the sun, (2) more distant objects at low galactic latitudes, and (3) objects at high galactic latitudes. Overall properties of the Galaxy and evolutionary effects are presented in Section IV.

Type
Other
Information
Transactions of the International Astronomical Union , Volume 19 , Issue 1 , 1985 , pp. 407 - 409
Copyright
Copyright © Reidel 1985

References

Feitzinger, J.V., Stüwe, J.A.: 1984, Astron. Astrophys. Suppl. (in preparation).Google Scholar
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Trefzger, Ch. F.: 1984, IAU Symposium No. 106 (in press).Google Scholar
Winkler, Chr., Schmidt-Kaler, Th., Schlosser, W.: 1984, Astron. Astrophys. Suppl,(submitted).Google Scholar