Possibilities and Attempts to Determine the Differential Rotation on F-Type Main-Sequence Stars

Symposium - International Astronomical Union
doi 10.1017/s0074180900029818
Full Text
Abstract

Available in full text

Date
Authors
Publisher

Cambridge University Press (CUP)

Related search

The Rotation of Pre-Main Sequence Stars

Highlights of Astronomy
1980English

Mathematical Assessment of Physical and Chemical Processes From the Middle B to the Early F Type Main Sequence Stars

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2017English

Magnetic Fields in O-, B- And A-Type Stars on the Main Sequence

EPJ Web of Conferences
AstronomyPhysics
2015English

Rotational Velocity Distributions of A-Type Main-Sequence Stars

Symposium - International Astronomical Union
2004English

Spectroscopic Evolution of Massive Stars on the Main Sequence

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2017English

Spectroscopic Investigation of Stars on the Lower Main Sequence

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2008English

Turbulence in Main Sequence Stars

International Astronomical Union Colloquium
1980English

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

Amanote Research

Note-taking for researchers

Follow Amanote

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

Privacy PolicyRefund Policy