Hostname: page-component-cd9895bd7-gbm5v Total loading time: 0 Render date: 2024-12-25T15:53:33.834Z Has data issue: false hasContentIssue false

Ultraviolet interstellar extinction from a comparison of Persei and ζ Persei

Published online by Cambridge University Press:  14 August 2015

Theodore P. Stecher*
Affiliation:
NASA, Goddard Space Flight Center, Greenbelt, 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.

Hall's and Stebbins and Whitford's extinction pair has been used to determine interstellar extinction in the ultraviolet. The extinction shows a feature suggestive of graphite. Previous observations of Stecher (1965) are confirmed. The results are presented in the figures.

Type
Part I: Stellar Fluxes
Copyright
Copyright © Reidel 1970 

References

Hall, J. S.: 1937, Astrophys. J. 85, 150.Google Scholar
Johnson, H. L., Mitchell, R. I., Iriate, B., and Wisniewski, W. Z.: 1966, Comm. of the Lunar and Planetary Laboratory 4, 99.Google Scholar
Stebbins, J. and Whitford, A. E.: 1943, Astrophys. J. 98, 20.CrossRefGoogle Scholar
Stebbins, J. and Whitford, A. E.: 1945, Astrophys. J. 102, 318.Google Scholar
Stecher, T. P.: 1965, Astrophys. J. 142, 1683.Google Scholar
Stecher, T. P.: 1969a, Astrophys. J. (in press).Google Scholar
Stecher, T. P.: 1969b, Astron. J. 74, 98.Google Scholar
Stecher, T. P. and Donn, B.: 1965, Astrophys. J. 142, 1681.Google Scholar
Stecher, T. P. and Williams, D. A.: 1969, Astrophys. Letters 4, 99.Google Scholar
Wickramasinghe, N. C. and Guillaumc, C.: 1965, Nature 207, 366.Google Scholar