Hostname: page-component-cd9895bd7-gbm5v Total loading time: 0 Render date: 2024-12-23T15:50:15.172Z Has data issue: false hasContentIssue false

Observations of Eclipsing Dwarf Novae

Published online by Cambridge University Press:  12 April 2016

J. Wood*
Affiliation:
Institute of Astronomy, Cambridge, U.K.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

High Speed Photometry of four eclipsing dwarf novae, Z Cha, OY Car, HT Cas and IP Peg, is used to determine the orbital parameters and the masses of the two stars in each system. The mass ratio, q, and inclination, i, are found by constraining theoretical stream trajectories (Lubow and Shu 1975) to pass through the observed light centre of the bright spot eclipse. The light centre is defined as the point corresponding to the half flux points in the ingress and egress of the eclipse of the compact part of the bright spot. The theoretical stream width indicates that the centre of the stream must intersect the bright spot close to this point.

Type
II. Radio, IR and Optical Observations
Copyright
Copyright © Reidel 1987

References

Horne, K.D., Wood, J.H., Stiening, R.P. 1987 Ap. J. in preparationGoogle Scholar
Lubow, S.H., Shu, F.H. 1975 Ap. J. 198, 383 Google Scholar
Martin, J.S., Jones, D.H.P.J., Smith, R.C. 1986 Mon. Not. R. astr. Soc. in pressGoogle Scholar
Wood, J.H., Horne, K.D., Berriman, G., Wade, R.A., O’Donoghue, D., Warner, B 1986 Mon. Not. R. astr. Soc. 219, 629 Google Scholar
Wood, J.H., Crawford, C.S. 1986 Mon. Not. R. astr. Soc in pressGoogle Scholar
Wood, J.H., Borne, K.D., Wade, R.A., Berriman, G. 1987 Mon. Not. R. astr. Soc. in preparationGoogle Scholar