Titlebook: Mass Loss from Stars; Proceedings of the S Margherita Hack Conference proceedings 1969 D. Reidel Publishing Company, Dordrecht, Holland 196

要塞

Possibility of Mass Loss in the Red-Giant Stage from H-R Diagrams of Galactic Clustersisochronous curves without mass loss derived from Iben’s evolutionary tracks and time scales for Population I stars. Interpreting the difference in magnitude between the theoretical positions thus calculated and the observed ones as due to mass loss, when negative, the results indicate that this los

公豬

Antarctic

finale

BABY

Coronae Around Helium Stars and X-Ray Sourcest log . = 4 and 15000K at log . = 6. The author’s suggestion in his last paper that a helium star . Sgr may have a corona seems to be justified. X-ray from a corona around a helium star is strongest when the physical parameters of the star are logg ~ 6 and T. ~ 15000K. But the total energy flux is t

Creditee

was primitive by today‘s standards, demonstrated the extraordinary potential of the NMR method. The subsequent rapid advances in this area were due largely to the ef- forts of commercial manufacturers, who, by improving magnet and computer designs, were able to produce and market instruments having

圓錐體

obtuse

變形詞

Anne B. Underhilldamit zu rechtfertigen, da? die Wechselwirkungen zwischen ungepaarten Elektronenspins und Kernen deutlich gr??er sind als zwischen den Kernen untereinander. Starke Verschiebungen und Aufspaltungen fallen auch in polykristallinen Proben auf. Hinzu kommt, da? eine regelm??ige und r?umlich dichte Anord

WAG