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Rotational Disturbance in BG CMi

  • M. A. Garlick
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 208)

Abstract

I report on the independent discovery of a feature in BG CMi which resembles a rotational disturbance (RD). A similar effect has already been reported in the He IIλ 4686 line, whereas here it ia seen in the Balmer lines, 0.25 orbital cycles prior to that reported previously. These results suggest that BG CMi is at a relatively high inclination.

Keywords

Accretion Disc White Dwarf Independent Discovery Orbital Phase Phase Zero 
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.

References

  1. Garlick, M.A., Rosen, S.R., Mittaz, J.P.D., et al., 1994, MNRAS, 267, 1095ADSGoogle Scholar
  2. Hellier, C., Garlick, M.A., Mason, K.O., 1993, MNRAS, 260, 299ADSGoogle Scholar
  3. de Martino, D., Mouchet, M., Bonnet-Bidaud, J.M., et al., 1995, A&Amp;A, 298, 849ADSGoogle Scholar
  4. Patterson, J., Thomas, G., 1993, PASP, 105, 59ADSCrossRefGoogle Scholar

Copyright information

© Kluwer Academic Publishers 1996

Authors and Affiliations

  • M. A. Garlick
    • 1
  1. 1.Astronomy CentreUniversity of SussexBrightonUK

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