Important Consequences of Atomic Diffusion Inside Main-Sequence Stars: Opacities, Extra-Mixing, Oscillations

EPJ Web of Conferences - France
doi 10.1051/epjconf/201715206007
Full Text
Abstract

Available in full text

Date
Authors
Publisher

EDP Sciences

Related search

Atomic Diffusion and Mixing in Old Stars

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2014English

Chemical Abundances of Main-Sequence, Turnoff, Subgiant, and Red Giant Stars From APOGEE Spectra. II. Atomic Diffusion in M67 Stars

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2019English

Role of Atomic Diffusion in the Opacity Enhancement Inside B-Type Stars

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2018English

Turbulence in Main Sequence Stars

International Astronomical Union Colloquium
1980English

Asteroseismology of Pre-Main Sequence Stars

Communications in Asteroseismology
2009English

Rotating Magnetic Upper-Main Sequence Stars

Bulletin of the Australian Mathematical Society
Mathematics
1985English

Thermohaline Convection in Main Sequence Stars

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2008English

The Rotation of Pre-Main Sequence Stars

Highlights of Astronomy
1980English

VINCI/VLTI Observations of Main Sequence Stars

Symposium - International Astronomical Union
2004English

Amanote Research

Note-taking for researchers

Follow Amanote

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

Privacy PolicyRefund Policy