Hostname: page-component-cd9895bd7-dk4vv Total loading time: 0 Render date: 2024-12-26T03:11:37.702Z Has data issue: false hasContentIssue false
  • English
  • Français

Galactic Dust Distribution in the Solar Neighborhood

Published online by Cambridge University Press:  14 August 2015

J. H. Cahn  and
R.D. Nosek
J. H. Cahn
Affiliation:
University of Illinois Observatory, Urbana, Ill. 61801, U.S.A.
R.D. Nosek
Affiliation:
University of Illinois Observatory, Urbana, Ill. 61801, 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.

Using the Shklovsky-Minkowski-Aller constant mass method of distances to planetary nebulae, a model of the Galactic dust distribution in the vicinity of the Sun has been determined. Distances are determined in part from extinctions derived from radio continuum to Hβ flux ratios for an assumed electron temperature of 7000 K. The distance scale is based on the brightness of planetary nebulae in the Magellanic Clouds (Seaton, 1968).

Type
Part V Distribution of Dust and Gas
Information
Symposium - International Astronomical Union , Volume 52: Interstellar Dust and Related Topics , 1973 , pp. 237 - 241
Copyright
Copyright © Reidel 1973 

References

Cahn, J. H. and Kaler, J. B.: 1971, Astrophys. J. Suppl 22, 319.CrossRefGoogle Scholar
Fitzgerald, M. Pim: 1968, Astron. J. 73, 983.CrossRefGoogle Scholar
Mills, B.: 1959, in Bracewell, R. N. (ed.), ‘Paris Symposium on Radio Astronomy’, IAU Symp. 9, 431.Google Scholar
Peimbert, M.: 1971, Bol. Obs. Tonantzintla Tacubaya 6, 29.Google Scholar
Seaton, M. J.: 1968, Astrophys. Letters 2, 55.Google Scholar
Simonson, S. C.: 1970, Astron. Astrophys. 9, 163.Google Scholar