'Strong temperature dependence' diaporamas de présentation

Stellar Evolution

0. Stellar Evolution. 0. Evolution on the Main Sequence. Development of an isothermal core:. dT/dr = (3/4ac) ( k r/T 3 ) (L r /4 p r 2 ). MS evolution. Zero-Age Main Sequence (ZAMS). L r = 0 => T = const. 0. Interior of a 1 M 0 Star. X H (4.3 x 10 9 yr). X H (9.2 x 10 9 yr).

235 views • 17 slides

164 views • 10 slides

Possibility of an application of High Tc bulk superconductor material

Possibility of an application of High Tc bulk superconductor material QMG(Quench and Melt Growth) to Final Doublet Mitsuru Morita, Nippon Steel Coporation, M. Kumada, NIRS.

142 views • 6 slides