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Rotational Disturbance in BG CMI

Published online by Cambridge University Press:  12 April 2016

M. A. Garlick
M. A. Garlick*
Affiliation:
Astronomy Centre, University of Sussex, Brighton BN1 9QH, UK

Abstract

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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 is 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.

Type
Intermediate Polars
Information
International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996 , pp. 179 - 180
Copyright
Copyright © Kluwer 1996

References

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