Properties of the main-sequence eclipsing binary AY Camelopardalis

Details Properties of the main-sequence eclipsing binary AY Camelopardalis Properties of the main-sequence eclipsing binary AY Camelopardalis

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987aj.....94.1670l&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 94, Dec. 1987, p. 1670-1672. NSF-supported research.

Astronomy and Astrophysics

Astronomy

5

Eclipsing Binary Stars, Line Shape, Main Sequence Stars, Radial Velocity, Stellar Evolution, Stellar Spectra, Light Curve, Stellar Cores, Stellar Models, Stellar Spectrophotometry

Scientific paper

Radial velocities and line profiles of AY Cam are analyzed, and the results are combined with previous light-curve analyses to yield absolute properties of this binary. Comparison of the properties of these stars with theoretical models of stellar evolution indicates that the primary component is significantly beyond the point of core-hydrogen exhaustion and the secondary is near the point of core-hydrogen exhaustion.

Affiliated with

Also associated with

No associations

Rating

Properties of the main-sequence eclipsing binary AY Camelopardalis 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 Properties of the main-sequence eclipsing binary AY Camelopardalis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Properties of the main-sequence eclipsing binary AY Camelopardalis will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-900762