The Influences of Convective Overshooting and Semiconvection on the Chemical Evolution of Massive Stars

Research in Astronomy and Astrophysics - United Kingdom
doi 10.1088/1674-4527/14/8/008
Full Text
Abstract

Available in full text

Date
Authors
Publisher

IOP Publishing

Related search

The S-Process Nucleosynthesis in Massive Stars: Current Status and Uncertainties Due to Convective Overshooting

2012English

The Evolution of Massive Stars

Symposium - International Astronomical Union
1997English

On the Evolution and Fate of Super-Massive Stars

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2007English

Spectroscopic Evolution of Massive Stars on the Main Sequence

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2017English

Convective Overshooting to Drive G-Modes in Γ Dor Stars

Symposium - International Astronomical Union
2001English

Evolution of Zero-Metallicity Massive Stars

Symposium - International Astronomical Union
2003English

Chemical Abundances of Fast-Rotating Massive Stars

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2017English

Evolution of Massive Stars After Helium Burning.

Astronomical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
1962English

Chemical Composition of Halo Field Stars and the Chemical Evolution of the Halo

Highlights of Astronomy
1983English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2024 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy