The Eclipsing Binary System V2154 Cyg : Observations and Models

Details The Eclipsing Binary System V2154 Cyg : Observations and Models The Eclipsing Binary System V2154 Cyg : Observations and Models

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007iaus..240..388f&link_type=abstract

Binary Stars as Critical Tools and Tests in Contemporary Astrophysics, International Astronomical Union. Symposium no. 240, he

Astronomy and Astrophysics

Astrophysics

Scientific paper

V2154 Cyg is one of the nearest eclipsing binary systems located at 88 pc and discovered by the HIPPARCOS mission. Based on photometric and spectroscopic observations carried out respectively at the Nevada Observatory, Spain (uvby photometry) and by CORAVEL-ELODIE , at the Haute-Provence Observatory, we determine the masses, effective temperature and radius for both components of the eclipsin system. On the other hand we analyse the HR Diagram position of V2154 Cyg A and B by means of the theoretical models. This system is very interesting thanks to the fact that, being composed by coeval stars, the different masses the eclipsing binary components (1.27Mo + 0.76 Mo) allow the comparison between two stars with clear different internal structures and evolutionary regimes, mainly on convection processes. We present preliminary results on the determination of the age and helium of the system.

Affiliated with

Also associated with

No associations

Rating

The Eclipsing Binary System V2154 Cyg : Observations and Models 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 The Eclipsing Binary System V2154 Cyg : Observations and Models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Eclipsing Binary System V2154 Cyg : Observations and Models will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1811085