Pulsation and mass loss for post-main sequence stars

Details Pulsation and mass loss for post-main sequence stars Pulsation and mass loss for post-main sequence stars

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986iraj...17..249w&link_type=abstract

Irish Astronomical Journal (ISSN 0021-1052), vol. 17, March 1986, p. 249-256.

Statistics

Computation

10

Main Sequence Stars, Stellar Mass Ejection, Stellar Models, Stellar Oscillations, Variable Stars, Computational Astrophysics, Hydrodynamics, Numerical Integration, Stellar Atmospheres

Scientific paper

The basis for this paper is an analysis of a number of numerical hydrodynamical models for the atmospheres of variable stars, mostly corresponding to the Miras and closely related long-period variables but including some preliminary models for RR Lyrae and Cepheid variables. Quantitative results are still tentative, but the qualitative picture which is emerging is quite encouraging for the hypothesis that pulsation leads to significant mass loss for a variety of stars.

Affiliated with

Also associated with

No associations

Rating

Pulsation and mass loss for post-main sequence 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 Pulsation and mass loss for post-main sequence stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Pulsation and mass loss for post-main sequence stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1282563