Abstract
In this paper the effect of complete homogenization in the intermediate unstable layers of massive stars is briefly discussed on the effective temperature of the core He-burning models. To this end, a 20 solar masses star of Population I chemical composition (X=0.700, Z=0.020) has been allowed to evolve from the Main Sequence into the core He-exhaustion stage without taking into account semiconvective mixing. The results show that the models are systematically bluer than those computed with the same physical parameters but with the inclusion of semiconvection.
Chiosi, C;
[1]
Nasi, E
[2]
- Padua Univ. (Italy). Ist. di Astronomia
- Osservatorio Astronomico, Padova, Italy
Citation Formats
Chiosi, C, and Nasi, E.
Convective shells and the core He-burning phase of massive stars.
Netherlands: N. p.,
1978.
Web.
doi:10.1007/BF01879574.
Chiosi, C, & Nasi, E.
Convective shells and the core He-burning phase of massive stars.
Netherlands.
https://doi.org/10.1007/BF01879574
Chiosi, C, and Nasi, E.
1978.
"Convective shells and the core He-burning phase of massive stars."
Netherlands.
https://doi.org/10.1007/BF01879574.
@misc{etde_6331742,
title = {Convective shells and the core He-burning phase of massive stars}
author = {Chiosi, C, and Nasi, E}
abstractNote = {In this paper the effect of complete homogenization in the intermediate unstable layers of massive stars is briefly discussed on the effective temperature of the core He-burning models. To this end, a 20 solar masses star of Population I chemical composition (X=0.700, Z=0.020) has been allowed to evolve from the Main Sequence into the core He-exhaustion stage without taking into account semiconvective mixing. The results show that the models are systematically bluer than those computed with the same physical parameters but with the inclusion of semiconvection.}
doi = {10.1007/BF01879574}
journal = []
volume = {56:2}
journal type = {AC}
place = {Netherlands}
year = {1978}
month = {Jul}
}
title = {Convective shells and the core He-burning phase of massive stars}
author = {Chiosi, C, and Nasi, E}
abstractNote = {In this paper the effect of complete homogenization in the intermediate unstable layers of massive stars is briefly discussed on the effective temperature of the core He-burning models. To this end, a 20 solar masses star of Population I chemical composition (X=0.700, Z=0.020) has been allowed to evolve from the Main Sequence into the core He-exhaustion stage without taking into account semiconvective mixing. The results show that the models are systematically bluer than those computed with the same physical parameters but with the inclusion of semiconvection.}
doi = {10.1007/BF01879574}
journal = []
volume = {56:2}
journal type = {AC}
place = {Netherlands}
year = {1978}
month = {Jul}
}