SpringerLink
Forum Springer Astron. Astrophys.
Forum Whats New Search Orders


Astron. Astrophys. 342, 704-708 (1999)

Previous Section Next Section Title Page Table of Contents

Acknowledgements

My thanks are due to U. Grabowski, who computed the hydrostatics of degenerate isothermal cores and to M. Stix who carried out the numerical simulations of the advanced solar evolution. The hospitality of the Instituto de Astrofisica de Canarias (La Laguna, Tenerife) is gratefully acknowledged, where this version of the paper was written down. Finally I am most grateful to E.E. Salpeter, who taught me several decades ago that all important phases of stellar evolution must be physically transparent on the basis of polytropic theory.

Previous Section Next Section Title Page Table of Contents

© European Southern Observatory (ESO) 1999

Online publication: February 23, 1999
helpdesk.link@springer.de