Accessibility navigation


Are superhumps good measures of the mass ratio for AM CVn systems?

Pearson, K. J. (2007) Are superhumps good measures of the mass ratio for AM CVn systems? Monthly Notices of the Royal Astronomical Society, 379 (1). pp. 183-189. ISSN 0035-8711

Full text not archived in this repository.

It is advisable to refer to the publisher's version if you intend to cite from this work. See Guidance on citing.

To link to this item DOI: 10.1111/j.1365-2966.2007.11932.x

Abstract/Summary

We extend recent work that included the effect of pressure forces to derive the precession rate of eccentric accretion discs in cataclysmic variables to the case of double degenerate systems. We find that the logical scaling of the pressure force in such systems results in predictions of unrealistically high primary masses. Using the prototype AM CVn as a calibrator for the magnitude of the effect, we find that there is no scaling that applies consistently to all the systems in the class. We discuss the reasons for the lack of a superhump period to mass ratio relationship analogous to that known for SU UMa systems and suggest that this is because these secondaries do not have a single valued mass-radius relationship. We highlight the unreliability of mass-ratios derived by applying the SU UMa expression to the AM CVn binaries.

Item Type:Article
Refereed:Yes
Divisions:No Reading authors. Back catalogue items
Science > School of Mathematical, Physical and Computational Sciences > Department of Meteorology
ID Code:34180
Publisher:Oxford Journals

University Staff: Request a correction | Centaur Editors: Update this record

Page navigation