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Extinction Maps of Dust Clouds from Surface Photometry

Published online by Cambridge University Press:  08 February 2017

K. J. Seidensticker  and
Th. Schmidt-Kaler
K. J. Seidensticker
Affiliation:
Astronomical Institute Ruhr-Universität Bochum Postfach 102148 D–4630 Bochum 1 FRG
Th. Schmidt-Kaler
Affiliation:
Astronomical Institute Ruhr-Universität Bochum Postfach 102148 D–4630 Bochum 1 FRG

Abstract

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We present a new method, based on surface photometry, which allows one to make the spatial resolution of extinction maps of dark clouds as fine as necessary. Applying this technique to the Coalsack (l = 302°, b = 0°), we derived an extinction map and the dust mass MD = (62 ± 25) M⊙. The density was found to vary ρ ~ r−0.8, typical for stable clouds.

Type
III. Diffuse Galactic Radiation from Dust and Gas: Observations and Models
Information
Symposium - International Astronomical Union , Volume 139: The Galactic and Extragalactic Background Radiation , 1990 , pp. 239 - 240
Copyright
Copyright © Kluwer 1990 

References

REFERENCES

Cernicharo, J., Bachiller, R., and Duvert, G. 1985, Astron. Astrophys., 149, 273.Google Scholar
Falgarone, E. and Puget, J. L. 1985, Astron. Astrophys., 142, 157.Google Scholar
Lillie, C. F. and Witt, A. N. 1976, Ap. J., 208, 64.Google Scholar
Mattila, K. 1970, Astron. Astrophys., 9, 53.Google Scholar
Mattila, K. 1976, Astron. Astrophys., 47, 77.Google Scholar
Seidensticker, K. J., Schmidt-Kaler, Th., and Schlosser, W. 1982, Astron. Astrophys., 114, 60.Google Scholar