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Observations of Interstellar HI Toward Nearby Late-Type Stars

Published online by Cambridge University Press:  12 April 2016

Wayne B. Landsman ,
Richard C. Henry ,
H. Warren Moos  and
Jeffrey L. Linsky
Wayne B. Landsman
Affiliation:
NASA/Goddard Space Flight Center
Richard C. Henry
Affiliation:
Johns Hopkins University
H. Warren Moos
Affiliation:
Johns Hopkins University
Jeffrey L. Linsky
Affiliation:
JILA, Universtiy of Colorado, and NBS

Abstract

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High-dispersion Copernicus and IUE observations of chromospheric Ly α emission are used to study the distribution of HI in the local interstellar medium. Interstellar parameters are derived toward 3 stars within 5 pc of the sun, and upper limits are given for the Ly a flux from 9 other stars within 10 pc.

Type
Ultraviolet and EUV Absorption Studies
Information
International Astronomical Union Colloquium , Volume 81: Local Interstellar Medium , 1984 , pp. 60 - 63
Copyright
Copyright © NASA 1984

References

Anderson, R.C., Henry, R.C., Moos, H.W., and Linsky, J.L. 1978, Ap.J., 226, 883.Google Scholar
Blanco, C., Catalano, S., Marilli, E. 1980, in Proceedings of the Second European IUE Conference, (ESA SP-157), p.63.Google Scholar
Crutcher, R.M. 1982, Ap. J., 254, 82.CrossRefGoogle Scholar
Landsman, W.B. 1984, Ph.D. Thesis, Johns Hopkins University.Google Scholar
Landsman, W.B., Henry, R.C., Moos, H.W., and Linsky, J.L. 1984, to be published in Ap. J. Google Scholar
McClintock, W. Henry, R.C., Linsky, J.L. and Moos, H.W. 1978, Ap. J., 202, 733.Google Scholar