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Eclipse Observations of IP Peg During Outburst

Published online by Cambridge University Press:  12 April 2016

W. J. Worraker ,
T. Naylor ,
G. Poyner  and
S. J. Robinson
W. J. Worraker
Affiliation:
British Astronomical Association, 65 Wantage Road, Didcot, Oxon., OX11 0AE, UK
T. Naylor
Affiliation:
Department of Physics, Keele University, Staffs, ST5 5BG, UK
G. Poyner
Affiliation:
British Astronomical Association, 67 Ellerton Road, Kingstanding, Birmingham, B44 0QE, UK
S. J. Robinson
Affiliation:
178 Fearns Avenue, Bradwell, Stoke-on-Trent, Staffs, UK

Extract

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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 Google Scholar
2. Skiff, B.A., 1994, VSNET message ‘Skiff on IP Peg, issued on 9th OctoberGoogle Scholar
3. Somers, M.W., Mukai, K., Naylor, T., 1996, MNRAS, in pressGoogle Scholar
4. VSNET postings, August 1994Google Scholar
5. Wood, J.H., Marsh, T.R., Robinson, E.L., et al., 1989, MNRAS, 239, 809 Google Scholar
6. Wood, J.H., Crawford, C.S., 1986, MNRAS, 222, 645 Google Scholar