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Space Observations of Chemically Peculiar and Related Normal Stars

Published online by Cambridge University Press:  12 April 2016

David S. Leckrone
David S. Leckrone*
Affiliation:
Laboratory for Astronomy and Solar Physics Goddard Space Flight Center Greenbelt, Maryland, USA

Abstract

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Progress in the spectroscopic study of CP stars and related sharp-lined normal stars from the IUE is briefly reviewed as a preamble to a discussion of the potential for research with the Hubble Space Telescope. The substantial gains in spectral resolution, signal-to-noise ratio and photometric accuracy that will be realized with the High Resolution Spectrograph on the HST will dramatically increase our ability to disentangle the complex ultraviolet spectra of these stars and to carry out accurate quantitative analyses.

Type
Section I - Theoretical Considerations
Information
International Astronomical Union Colloquium , Volume 90: Upper Main Sequence Stars with Anomalous Abundances , 1986 , pp. 109 - 119
Copyright
Copyright © Reidel 1986

References

Adelman, S.J. and Leckrone, D.S. 1985, NASA IUE Newsletter, No. 28, in press.Google Scholar
Dworetsky, M.M., Storey, P.J. and Jacobs, J.M. 1984, Physica Scrlpta, T8, p. 39.Google Scholar
Jacobs, J.M. and Dworetsky, M.M. 1981, in Upper Main Sequence Chemically Peculiar Stars, 23r Liege International Astrophysical Colloquium, p. 153.Google Scholar
Jacobs, J.M. and Dworetsky, M.M. 1982, Nature, 299, p. 535.Google Scholar
Kurucz, R.L. 1981, Smithsonian Astrophysical Obs. Special Report, No. 390.Google Scholar
Kurucz, R.L. and Peytremann, E. 1975, Smithsonian Astrophysical Obs. Special Report, No. 362.Google Scholar
Leckrone, D.S. 1975, in Physics of Ap-Stars, IAU Coll. No. 32, (ed., Weiss, W., Jenkner, H. and Wood, H.), University of Vienna, p. 465.Google Scholar
Leckrone, D.S. 1980, Highlights of Astr., 5, p. 277.Google Scholar
Leckrone, D.S. 1981, Astrophys. J., 250, p. 687.Google Scholar
Leckrone, D.S. 1984, Astrophys. J., 286, p. 725.Google Scholar
Martin, G.A., Fuhr, J.R. and Wiese, W.L. 1986, in preparation.Google Scholar
Sadakane, K., Takada, M. and Jugaku, J. 1983, Astrophys. J., 274, p. 261.Google Scholar
Sadakane, K., Jugaku, J. and Takada-Hidai, M. 1985, Astrophys. J., 297, p. 240.Google Scholar