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Gas and Dust in Interstellar Clouds

Published online by Cambridge University Press:  14 August 2015

R. D. Davies
R. D. Davies*
Affiliation:
University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank, U.K.

Abstract

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Detailed measurements have been made of the H, OH and H2CO lines formed in the L1534 dense dust cloud; some H and H2CO observations have been made of the dust cloud lying behind the Orion cluster. These indicate a similar distribution of the 3 species throughout the dust clouds. Studies of H, OH and H2CO absorption features in clouds lying in front of bright radio sources provide estimates of the physical conditions in regions of molecule formation.

Type
Part V Distribution of Dust and Gas
Information
Symposium - International Astronomical Union , Volume 52: Interstellar Dust and Related Topics , 1973 , pp. 251 - 255
Copyright
Copyright © Reidel 1973 

References

Cohen, R. J., Davies, R. D., and Wilson, A. J.: 1972, in preparation. Google Scholar
Davies, R. D. and Matthews, H. E.: 1972, Monthly Notices Roy. Astron. Soc. 156, 253.CrossRefGoogle Scholar
Heiles, C.: 1968, Astrophys. J. 151, 919.CrossRefGoogle Scholar
Heiles, C.: 1970, Astrophys. J. 160, 51.CrossRefGoogle Scholar
Hollenbach, D. J., Werner, M. W., and Salpeter, E. E.: 1971, Astrophys. J. 163, 165.CrossRefGoogle Scholar
Kutner, M. and Thaddeus, P.: 1971, Astrophys. J. 168, L67.CrossRefGoogle Scholar
Lynds, B. T.: 1962, Astrophys. J. Suppl. 7, 1.CrossRefGoogle Scholar
Palmer, P., Zuckerman, B., Buhl, D., and Snyder, L. E.: 1969, Astrophys. J. 156, L147.CrossRefGoogle Scholar