Variability of long-period pulsating stars. III. Changes in the parameters of humps at the ascending branch

Details Variability of long-period pulsating stars. III. Changes in the parameters of humps at the ascending branch Variability of long-period pulsating stars. III. Changes in the parameters of humps at the ascending branch

Jan 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ap.....50...76m&link_type=abstract

Astrophysics, Volume 50, Issue 1, pp.76-82

Astronomy and Astrophysics

Astrophysics

Stars, Long Period Variables, Light Curves

Scientific paper

The properties of such phenomena as the appearance of humps at the ascending branch or double peaks in the light curve of long-period pulsating stars are examined. The characteristics of humps and the average light curves are obtained for a group of Mira-type stars and semiregular (SRa) variable stars. Correlations between the parameters of the light curves and the characteristics of the humps for these stars are discussed. The results obtained here are compared with published theoretical models.

Affiliated with

Also associated with

No associations

Rating

Variability of long-period pulsating stars. III. Changes in the parameters of humps at the ascending branch 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 Variability of long-period pulsating stars. III. Changes in the parameters of humps at the ascending branch, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Variability of long-period pulsating stars. III. Changes in the parameters of humps at the ascending branch will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1363940