Generation of Longitudinal Flux Tube Waves in Theoretical Main-Sequence Stars: Effects of Model Parameters

Astronomy and Astrophysics - France
doi 10.1051/0004-6361/201015250
Full Text
Abstract

Available in full text

Date
Authors
Publisher

EDP Sciences

Related search

Turbulence in Main Sequence Stars

International Astronomical Union Colloquium
1980English

Asteroseismology of Pre-Main Sequence Stars

Communications in Asteroseismology
2009English

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

Abundance Anomalies in Pre-Main-Sequence Stars

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2010English

Pre-Main Sequence Stars in Open Clusters

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2007English

Rotating Magnetic Upper-Main Sequence Stars

Bulletin of the Australian Mathematical Society
Mathematics
1985English

Photometric Detection of Internal Gravity Waves in Upper Main-Sequence Stars. I. Methodology and Application to CoRoT Targets

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2019English

Amanote Research

Note-taking for researchers

Follow Amanote

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

Privacy PolicyRefund Policy