Derivation of the Rotational Frequency of Massive Stars From Seismic Studies

Symposium - International Astronomical Union
doi 10.1017/s0074180900195543
Full Text
Abstract

Available in full text

Date
Authors
Publisher

Cambridge University Press (CUP)

Related search

On the Maximum Rotational Frequency of Neutron and Hybrid Stars

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2003English

The Stability of Massive Stars

Symposium - International Astronomical Union
1994English

Detailed Nucleosynthesis Yields From the Explosion of Massive Stars

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2007English

The Evolution of Massive Stars

Symposium - International Astronomical Union
1997English

The Influence of Feedback From Massive Stars on the Formation and Emergence of Massive Clusters

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2015English

The Derivation of the Rotational Potential Function From Atom–atom Potentials. III. Borohydride Compounds

Canadian Journal of Chemistry
Organic ChemistryCatalysisChemistry
1988English

Variability of Massive Stars in M31 From the Palomar Transient Factory

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2020English

Rotational Periods of Four roAp Stars

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2005English

The Physics of Convection in Massive Stars

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2014English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2025 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy