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A New High-Resolution Optical Study of Halo Gas

Published online by Cambridge University Press:  12 April 2016

C. E. Albert
Affiliation:
U.S. Naval Academy, Annapolis, MD, USA
J. C. Blades
Affiliation:
Space Telescope Science Institute, Baltimore, MD, USA
D. C. Morton
Affiliation:
Herzberg Institute of Astrophysics, Ottawa, ON, Canada
M. Proulx
Affiliation:
Herzberg Institute of Astrophysics, Ottawa, ON, Canada
F. J. Lockman
Affiliation:
National Radio Astronomy Observatory, Charlottesville, VA, USA

Abstract:

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We present preliminary results from a new high resolution optical study of halo gas at the coudé focus of the Canada - France - Hawaii Telescope. Our work is still in progress so two general results are presented here: significant absorption is produced in interstellar gas beyond 500 pc from the galactic plane, and well-resolved halo clouds are identified.

Type
VI. Interstellar Matter at High Galactic Latitudes
Copyright
Copyright © Springer-Verlag 1989

References

Albert, C. E. 1983, Ap.J., 272, 509.Google Scholar
Cohen, J. G., and Meloy, D.A. 1975, Ap.J., 198, 545.Google Scholar
Danly, L. 1989, this volume.Google Scholar
Greenstein, J. L. 1968, Ap.J., 152, 431.Google Scholar
Hulsbosch, A. N. M., and Wakker, B. P. 1988, Astr. Ap. Suppl. Ser., 75, 191.Google Scholar
Morton, D. C., and Blades, J. C. 1986, Mon. Not. R. astr. Soc., 220, 927.Google Scholar
Münch, G., and Zirin, H. 1961, Ap.J., 131, 11.Google Scholar
Richstone, D. O., and Morton, D. C. 1975, Ap. J., 201, 289.Google Scholar
Rickard, J. J. 1972, Astr. Ap., 17, 425.Google Scholar
Wakker, B. 1989, this volume.Google Scholar
Wallerstein, G., and Goldsmith, D. 1974, Ap.J., 187, 237.CrossRefGoogle Scholar