Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-11-25T17:58:32.273Z Has data issue: false hasContentIssue false
  • English
  • Français

The Gas-to-Dust Ratio in the Galaxy

Published online by Cambridge University Press:  14 August 2015

F. J. Kerr  and
G. R. Knapp
F. J. Kerr
Affiliation:
University of Maryland, College Park, Md., U.S.A.
G. R. Knapp
Affiliation:
University of Maryland, College Park, Md., U.S.A.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have investigated the gas-to-dust ratio in the Galaxy by comparing 21-cm Hicolumn densities with the color excesses of globular clusters. We find a constant gas-to-reddening ratio in interstellar clouds and the intercloud medium. This ratio is also independent of galactic latitude.

Type
Part 1: The Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 60: Galactic Radio Astronomy , 1974 , pp. 179 - 182
Copyright
Copyright © Reidel 1974 

References

Knapp, G. R., Kerr, F. J., and Rose, W. K.: 1973, Astrophys. Letters 14, 187.Google Scholar
Savage, B. D. and Jenkins, E. B.: 1972, Astrophys. J. 172, 491.CrossRefGoogle Scholar
Sturch, C.: 1969, Astron. J. 74, 82.CrossRefGoogle Scholar
van den Bergh, S.: Astron. J. 72, 70.CrossRefGoogle Scholar