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Dust in the Large Magellanic Cloud

Published online by Cambridge University Press:  14 August 2015

Hugh M. Johnson
Hugh M. Johnson*
Affiliation:
Lockheed Missiles and Space Company, Palo Alto, Calif., U.S.A.

Abstract

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A brief review of extinction effects is followed by a discussion of new Cerro Tololo Schmidt plates. They were exposed on parts of the LMC with filters which reveal the presence or absence of a continuum, such as one scattered on dust, in H ii regions. The results are presented in comparison with the Orion nebula which was observed in the same way. The continuum is always relatively weak in those LMC H ii regions which are significantly larger than Orion, but the continuum averages strong in the Orion-class and point-image nebulae.

Information

Type
Part VIII Dust and H II Regions
Information
Symposium - International Astronomical Union , Volume 52: Interstellar Dust and Related Topics , 1973, pp. 471 - 476
Copyright
Copyright © Reidel 1973 

References

Bok, B. J.: 1966, Ann. Rev. Astron. Astrophys. 4, 95.Google Scholar
Brück, M. T., Lawrence, L. C., Nandy, K. N., Thackeray, A. D., and Wood, R.: 1970, Nature 225, 532.Google Scholar
Dickel, H. R.: 1965, Astrophys. J. 141, 1306.Google Scholar
Dickel, H. R., Aller, L. H., and Faulkner, D. J.: 1964, in Kerr, F. J. and Rodgers, A. W. (eds.), The Galaxy and the Magellanic Clouds , Australian Acad. Sci., Canberra, p. 294.Google Scholar
Doherty, L., Henize, K. G., and Aller, L. H.: 1956, Astrophys. J. Suppl. 2, 345.Google Scholar
Henize, K. G.: 1956, Astrophys. J. Suppl. 2, 315.Google Scholar
Hodge, P. W.: 1972, Publ. Astron. Soc. Pacific 84, 365.Google Scholar
Johnson, H. M.: 1971, in Muller, A. B. (ed.), The Magellanic Clouds , D. Reidel Publ. Co., Dordrecht-Holland, p. 95.Google Scholar
Johnson, H. M.: 1968, in Middlehurst, B. M. and Aller, L. H. (eds.), Nebulae and Interstellar Matter , University of Chicago Press, Chicago, p. 63.Google Scholar
Lissberger, P. H. and Wilcock, W. L.: 1959, J. Opt. Soc. Am. 49, 126.CrossRefGoogle Scholar
Mathewson, D. S. and Healey, J. R.: 1964, in Kerr, F. J. and Rodgers, A. W. (eds.), The Galaxy and the Magellanic Clouds , Australian Acad. Sci., Canberra, p. 283.Google Scholar
O'Dell, C. R. and Hubbard, W. B.: 1965, Astrophys. J. 142, 591.Google Scholar
Pottasch, S. R.: Vistas in Astronomy 6, 149.CrossRefGoogle Scholar
Reddish, V. C.: 1968, Observatory 88, 139.Google Scholar
Shapley, H.: 1951, Proc. Nat. Acad. Sci. 37, 136.Google Scholar
Thackeray, A. D.: 1963, Adv. Astron. Astrophys. 2, 264.Google Scholar
Visvanathan, N.: 1966, Monthly Notices Roy. Astron. Soc. 132, 423.Google Scholar