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Eclipse Observations of IP Peg During Outburst
Published online by Cambridge University Press: 12 April 2016
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IP Peg is a U Gem-type dwarf nova with a very high orbital inclination such that the secondary star eclipses the white dwarf primary, accretion disc and hot spot in each orbit. An observing project was set up by ‘The Astronomer’ (TA) magazine and the British Astronomical Association Variable Star Section to make visual and CCD eclipse observations of IP Peg during outbursts in the 1994/95 season.
- Type
- Non-Magnetic Cataclysmic Variables
- Information
- International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996 , pp. 65 - 70
- Copyright
- Copyright © Kluwer 1996
References
1.
Frank, J., King, A.R., Raine, D.J., 1992, “Accretion Power in Astrophysics” (2nd Edition), Cambridge University Press
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4. VSNET postings, August 1994Google Scholar
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