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A Fuse Survey of Disk-Accreting Cataclysmic Variables

Published online by Cambridge University Press:  22 February 2018

C. S. Froning ,
K. S. Long ,
P. Szkody  and
B. T. Gänsicke
C. S. Froning
Affiliation:
CASA, University of Colorado, 389 UCB, Boulder, CO 80309USA (cfroning@casa.colorado.edu)
K. S. Long
Affiliation:
STSci, 3700 San Martin Dr., Baltimore, MD 21218USA (long@stsci.edu)
P. Szkody
Affiliation:
Astronomy Dept., Univ. of Washington, Seattle, WA 98195USA (szkody@astro.washington.edu)
B. T. Gänsicke
Affiliation:
Dept. of Physics and Astronomy, Univ. of Southampton, Highfield, Southampton SO17 1BJUK (btg@astro.soton.ac.uk)

Extract

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We present initial results of a survey of the FUV spectra of disk-accreting cataclysmic variables obtained with the Far Ultraviolet Spectroscopic Explorer (FUSE).

FUSE covers the 905 - 1188 Å range at spectral resolutions ≃0.1 Å. To date, FUSE has observed more than 65 cataclysmic variables (CVs). Publicly-available data include observations of 11 dwarf novae (DN), 15 non-magnetic novalikes (NLs), 7 intermediate polars and DQ Her stars, at least 15 polars, and 4 super-soft X-ray binaries.

Type
The Contributed Papers
Information
International Astronomical Union Colloquium , Volume 194: Compact binaries in the galaxy and beyond , 2004 , pp. 251
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

References

Froning, C. S., et al. 2003, Ap.J, 584, 433 Google Scholar
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Long, K. S., et al. 2003, Ap.J, 591, 1172 CrossRefGoogle Scholar
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