Temperature And Brightness Variations On Betelgeuse
Instrumentation And Research Programmes For Small Telescopes
Changes in TiO band strengths correlate well with the brightness changes of α Orionis, thus supporting the hypothesis of Schwarzschild that the irregular luminosity variations of red giants are due to temperature changes in a few extremely large convective elements on their surface.
J. B. Hearnshaw And P. L. Cottrell
118th Symposium of the International Astronomical Union
December 2-6, 1985
Christchurch, New Zealand
John E. Gaustad.
"Temperature And Brightness Variations On Betelgeuse".
Instrumentation And Research Programmes For Small Telescopes.