Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...127..309h&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 127, no. 2, Nov. 1983, p. 309-312.
Astronomy and Astrophysics
Astrophysics
20
Cepheid Variables, Hertzsprung-Russell Diagram, Mass Transfer, Stellar Evolution, Stellar Mass, Stellar Spectra, Convection, H Lines, Main Sequence Stars, Red Giant Stars
Scientific paper
In addition to the calculations presented and discussed in Paper I (Matraka et al., 1982), evolutionary calculations have been carried out for an extreme Population I star of total mass 5 solar masses. Overshooting at the border of the convective core during central H-burning is taken into account using two different values (0.5 and 1) of the ratio alpha (i) of mixing length to pressure scale height in the interior. For both of these sequences, the evolution through the red giant region is then calculated assuming a variety of values (0.5. . . 1.7) for alpha (0), which denotes the corresponding mixing length ratio in the outer convective zone. A variation of alpha (0) changes the penetration depth of the outer convective zone in a characteristic way; alpha (0) determines therefore the resulting X-profile which in turn influences the length of the loop in the H-R diagram. For overshooting with alpha (i) = 1, the loop does not cross the Cepheid strip unless alpha (0) is reduced to less than 0.5. Such crossings occur, however, for alpha (i) = alpha (0) = 0.5 (and possibly up to 0.7). Larger overshooting could be allowed without a suppression of the Cepheid phase, when smaller concentrations of the heavy elements were assumed, which is known to give larger loops.
Huang Run-Qian
Weigert A.
No associations
LandOfFree
Overshooting from convective cores and the occurrence of loops in the HRD. II - Evolution of 5 solar masses stars to the Cepheid phase 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 Overshooting from convective cores and the occurrence of loops in the HRD. II - Evolution of 5 solar masses stars to the Cepheid phase, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Overshooting from convective cores and the occurrence of loops in the HRD. II - Evolution of 5 solar masses stars to the Cepheid phase will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1483691