Work and Power for Rotational Motion
Binary Fission
Binary Fission
Shock Waves
Power
Kinematic Equations for Rotation
You might also read
Articles linked to this work by shared authors, journal, and citation graph.
Updated: Feb 12, 2026

Uncoupling Coriolis Force and Rotating Buoyancy Effects on Full-Field Heat Transfer Properties of a Rotating Channel
Published on: October 5, 2018
Zorawar Wadiasingh1, Alice K Harding2, Christo Venter1
1Centre for Space Research, North-West University, Potchefstroom, South Africa.
This study reveals two distinct modes in black widow and redback millisecond pulsar binaries, explaining their radio and X-ray emissions through intrabinary shock orientation and Doppler boosting.
Area of Science:
Background:
Purpose of the Study:
Main Methods:
Main Results:
Conclusions: