Bump Masses and Radii of Bl-Herculis Variables

Details Bump Masses and Radii of Bl-Herculis Variables Bump Masses and Radii of Bl-Herculis Variables

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ssrv...27..495p&link_type=abstract

Space Science Reviews, Volume 27, Issue 3-4, pp. 495-501

Physics

6

Scientific paper

Bump masses and radii are derived for 18 BL Her stars from the observed bump phase and the accurately known fundamental period. The mean mass M/M&sun; = 0.60 ± 0.09 agrees precisely with predictions from standard stellar evolution theory and gives a new test of the theoretical models. The derived radius of V553 Centauri is in good agreement with the radius recently determined by an independent modified Baade-Wesselink method by Balona. Finally, a preliminary discussion of possible continuations of the BL Her bump progression is given.

Affiliated with

Also associated with

No associations

Rating

Bump Masses and Radii of Bl-Herculis Variables 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 Bump Masses and Radii of Bl-Herculis Variables, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Bump Masses and Radii of Bl-Herculis Variables will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1392517