Titlebook: Mass Outflows from Stars and Galactic Nuclei; Proceedings of the S Luciana Bianchi,Roberto Gilmozzi Conference proceedings 1988 Kluwer Acad

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Quasi-Steady Outflows from Astrophysical Objects: Complementary Views from Different Experiencesh theorists and experimentalists, on the problem of mass outflows from astrophysical objects. We illustrate some of the principal physical similarities and differences between outflows in various astrophysical systems, and show how experiences derived from different subject areas can help to build a

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Properties of Winds and Chromospheres in G to M Giants and Supergiantsray and UV satellites. In particular, it is demonstrated that in Zeta Aur type eclipsing binaries, where a B star moves within the wind of a K or G supergiant, the B star can be used as a light source which probes the wind and extended chromosphere of the cool super-giant with spatial resolution. It

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Masses of Planetary Nebulae and their Central Stars the Magellanic Clouds or the galactic bulge are used, together with a sample of galactic nebulea whose distance is known from independent consideration. It is found that there is a general relationship between the nebular mass and its size. There is considerable real scatter in this relationship. T

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Mass Loss and Post-Asymptotic Giant-Branch Evolution(within ~ 2 or 3 × 10. yr) through the planetary nebulae (PN) phase. Considerable progress in our understanding of this post-asymptotic giant-branch (PAGB) evolution has been made during the last years since consistent computations through the AGB, with thermal pulses and mass loss taken into accoun

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