4. Non-Stable Magneto-Hydrodynamical Processes in Stars

Symposium - International Astronomical Union
doi 10.1017/s0074180900237601
Full Text
Abstract

Available in full text

Date
Authors
Publisher

Cambridge University Press (CUP)

Related search

APEX Observations of Non-Stationary Magneto-Hydrodynamical Shocks in W44

2015English

Spectra From Three-Dimensional Magneto-Hydrodynamical Accretion Flows

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2004English

Three-Dimensional Hydrodynamical CO5BOLD Model Atmospheres of Red Giant Stars

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2012English

Square Processes of Stable Processes

Advances in Applied Mathematics
2018English

A Hydrodynamical Model of the Circumstellar Bubble Created by Two Massive Stars

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2012English

Generic Conditions for Stable Hybrid Stars

2014English

Equilibrium Systems of Stable Processes

Pacific Journal of Mathematics
Mathematics
1967English

Stable Processes and Integral Equations

Transactions of the American Mathematical Society
MathematicsApplied Mathematics
1961English

2D Wind Clumping in Hot, Massive Stars From Hydrodynamical Line-Driven Instability Simulations Using a Pseudo-Planar Approach

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2018English

Amanote Research

Note-taking for researchers

Follow Amanote

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

Privacy PolicyRefund Policy