Spurious Eccentricities of Distorted Binary Components

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

14 pp, 2 tables, 12 fig; under review by ApJ

Scientific paper

10.1086/588270

I discuss the effect of physical distortion on the velocities of close binary components and how we may use the resulting distortion of velocity curves to constrain some properties of binary systems, such as inclination and mass ratio. Precise new velocities for 5 Cet convincingly detect these distortions with their theoretically predicted phase dependence. We can even use such distortions of velocity curves to test Lucy's theory of convective gravity darkening. The observed distortions for TT Hya and 5 Cet require the contact components of those systems to be gravity darkened, probably somewhat more than predicted by Lucy's theory but clearly not as much as expected for a radiative star. These results imply there is no credible evidence for eccentric orbits in binaries with contact components. I also present some speculative analyses of the observed properties of a binary encased in a non-rotating common envelope, if such an object could actually exist, and discuss how the limb darkening of some recently calculated model atmospheres for giant stars may bias my resuts for velocity-curve distortions, as well as other results from a wide range of analyses of binary stars.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Spurious Eccentricities of Distorted Binary Components does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Spurious Eccentricities of Distorted Binary Components, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spurious Eccentricities of Distorted Binary Components will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-338788

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.