Stellar evolution with turbuelnt diffusion mixing. IV Intermediate and low mass stars and C-12/C-13 ratio in giants of the first ascending branch

Details Stellar evolution with turbuelnt diffusion mixing. IV Intermediate and low mass stars and C-12/C-13 ratio in giants of the first ascending branch Stellar evolution with turbuelnt diffusion mixing. IV Intermediate and low mass stars and C-12/C-13 ratio in giants of the first ascending branch

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...131..316b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 131, no. 2, Feb. 1984, p. 316-326.

Astronomy and Astrophysics

Astrophysics

13

Carbon 12, Main Sequence Stars, Red Giant Stars, Stellar Evolution, Stellar Mass, Turbulent Diffusion, Turbulent Mixing, Abundance, Carbon 13, Molecular Weight, Radial Distribution, Stellar Models

Scientific paper

It has been suggested that mild turbulence is present in the radiative zones of rotating stars. Such turbulence has the effect to modify the surface abundance of processed elements. Stellar evolution in stars with masses in the range from one to three solar masses is considered, and an attempt is made to solve the puzzle of surface abundances (Li and Be in main sequence stars and C-12/C-13, C/N ratios in giants) by a unique physical process, turbulent diffusion. Attention is given to instabilities and turbulent mixing, the method employed for numerical simulations, stellar models with and without turbulent diffusion, semistationary models with inhibition of the diffusion, and a 1.5 solar mass model. The comparison of the considered models with red giants at the first dredge-up confirms the idea of turbulent transport during the life near the main sequence.

Affiliated with

Also associated with

No associations

Rating

Stellar evolution with turbuelnt diffusion mixing. IV Intermediate and low mass stars and C-12/C-13 ratio in giants of the first 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 Stellar evolution with turbuelnt diffusion mixing. IV Intermediate and low mass stars and C-12/C-13 ratio in giants of the first ascending branch, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stellar evolution with turbuelnt diffusion mixing. IV Intermediate and low mass stars and C-12/C-13 ratio in giants of the first ascending branch will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1857189