Eclipse Observations of IP Peg During Outburst

  • W. J. Worraker
  • T. Naylor
  • G. Poyner
  • S. J. Robinson
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 208)

Abstract

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.

Keywords

Accretion Disc Light Curf White Dwarf Visual Estimate Minimum Light 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

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    Frank, J., King, A.R., Raine, D.J., 1992, “Accretion Power in Astrophysics” (2nd Edition), Cambridge University PressGoogle Scholar
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    Skiff, B.A., 1994, VSNET message Skiff on IP Peg, issued on 9th OctoberGoogle Scholar
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    Somers, M. W., Mukai, K., Naylor, T., 1996, MNRAS, in pressGoogle Scholar
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    Wood, J. H., Crawford, C. S., 1986, MNRAS, 222, 645ADSGoogle Scholar

Copyright information

© Kluwer Academic Publishers 1996

Authors and Affiliations

  • W. J. Worraker
    • 1
  • T. Naylor
    • 2
  • G. Poyner
    • 3
  • S. J. Robinson
    • 4
  1. 1.British Astronomical AssociationOxonUK
  2. 2.Department of PhysicsKeele UniversityStaffsUK
  3. 3.British Astronomical AssociationBirminghamUK
  4. 4.BradwellStoke-on-Trent, StaffsUK

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