Comparison between standard evolution models for high amplitude δ Sct stars.

Details Comparison between standard evolution models for high amplitude δ Sct stars. Comparison between standard evolution models for high amplitude δ Sct stars.

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990rmxaa..21..389c&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica, Vol. 21, p. 389 - 390

Astronomy and Astrophysics

Astronomy

4

Delta Scuti Stars: Stellar Evolution, Delta Scuti Stars: Stroemgren Photometry

Scientific paper

Recent ubvyβ observations of high amplitude δ Sct stars obtained at Sierra Nevada (Spain) and La Silla (Chile) observatories are compared with standard evolution models. The authors find very good agreement between Claret et al. model's (1989) and those from Vanden Berg (1985). However, a systematic effect on the derived masses is found if one uses the Hejlesen's results as indicated by previous work by Andersen et al. (1984). The results derived from the evolution models are compared with those derived from pulsation theory. A good agreement is found.

Affiliated with

Also associated with

No associations

Rating

Comparison between standard evolution models for high amplitude δ Sct stars. 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 Comparison between standard evolution models for high amplitude δ Sct stars., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Comparison between standard evolution models for high amplitude δ Sct stars. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-843861