Hostname: page-component-78c5997874-94fs2 Total loading time: 0 Render date: 2024-11-14T06:37:20.036Z Has data issue: false hasContentIssue false
  • English
  • Français

Determining the Masses and Evolution of CVs through Ellipsoidal Variations

Published online by Cambridge University Press:  22 February 2018

Heather L. Osborne ,
Thomas E. Harrison ,
Joni J. Johnson  and
Steve B. Howell
Heather L. Osborne
Affiliation:
Department of Astronomy, New Mexico State University, Las Cruces, NM
Thomas E. Harrison
Affiliation:
Department of Astronomy, New Mexico State University, Las Cruces, NM
Joni J. Johnson
Affiliation:
Department of Astronomy, New Mexico State University, Las Cruces, NM
Steve B. Howell
Affiliation:
National Optical Astronomical Observatory

Extract

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.

We use simultaneous multi-wavelength BVRI-JHK photometric observations of cataclysmic variables (CVs) to determine the inclination angles of the systems, together with phase-resolved spectroscopy to calculate the K2 and vsini. We then calculate the masses of the system components. We are using these data to construct mass-radius diagrams of the secondaries in an effort to resolve some of the debate over their evolutionary history.

Type
The Contributed Papers
Information
International Astronomical Union Colloquium , Volume 194: Compact binaries in the galaxy and beyond , 2004 , pp. 250
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

References

Harrison, Т.E., et. al., 2004, this proceedingsGoogle Scholar
Howell, S.B., Nelson, L.A., & Rappaport, S. 2001, ApJ, 550, 89 Google Scholar