The evolutionary status of the pulsating helium star BD + 13 deg 3224 (V652 Her)

Details The evolutionary status of the pulsating helium star BD + 13 deg 3224 (V652 Her) The evolutionary status of the pulsating helium star BD + 13 deg 3224 (V652 Her)

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.210..731j&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 210, Oct. 1, 1984, p. 731-743. Research supported by th

Astronomy and Astrophysics

Astronomy

18

B Stars, Horizontal Branch Stars, Stellar Evolution, Stellar Models, Variable Stars, Abundance, Main Sequence Stars, Radiant Flux Density, Stellar Envelopes, Stellar Luminosity, Stellar Temperature, Surface Temperature

Scientific paper

Zero-age models and evolutionary sequences for horizontal-branch stars with very low envelope hydrogen abundances (X less than 0.01) have been constructed. Models with a helium core mass of 0.475 solar mass reproduce the observed luminosity and surface temperature of the pulsating helium star BD + 13 deg 3224 (V652 Her) very well. The rate of period decrease of BD + 13 deg 3224 can also be reproduced by considering the contraction of the models as they evolve from their zero-age position towards the Helium Main Sequence.

Affiliated with

Also associated with

No associations

Rating

The evolutionary status of the pulsating helium star BD + 13 deg 3224 (V652 Her) 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 evolutionary status of the pulsating helium star BD + 13 deg 3224 (V652 Her), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The evolutionary status of the pulsating helium star BD + 13 deg 3224 (V652 Her) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1229232