Amanote Research

Amanote Research

    RegisterSign In

Solar Oblateness and Differentially Rotating Polytropes

International Astronomical Union Colloquium
doi 10.1017/s0252921100027366
Full Text
Open PDF
Abstract

Available in full text

Date

January 1, 1970

Authors
G. G. FahlmanM. D. T. NaylorS. P. S. Anand
Publisher

Cambridge University Press (CUP)


Related search

3D Collapse and Accretion in Slowly Rotating Polytropes

2011English

A Numerical Study of the Fission Hypothesis for Rotating Polytropes

International Astronomical Union Colloquium
1980English

Eigenoscillations of the Differentially Rotating Sun

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2004English

Differentially Heated Flow From a Rotating Sphere

2014English

Eclipse Intervals for Satellites in Circular Orbit Under the Effects of Earth’s Oblateness and Solar Radiation Pressure

NRIAG Journal of Astronomy and Geophysics
2015English

Discontinuity Modes in Polytropes

International Astronomical Union Colloquium
1989English

Yields of Rotating Stars at Solar Metallicity

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2005English

Global Numerical Simulations of Differentially Rotating Disks With Free Eccentricity

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2005English

Solar Heating of a Rotating Solid Cylinder

Quarterly of Applied Mathematics
Applied Mathematics
1963English

Amanote Research

Note-taking for researchers

Follow Amanote

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

Privacy PolicyRefund Policy