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

縮減了

Mechanisms for Outflow in AGNs (~ 0.26 c) suggests that radiative acceleration may be responsible; but there are difficulties with this interpretation, and it is perhaps unlikely that analogous effects occur in AGNs. In the pair-dominated plasmas expected in AGNs, radiation pressure is competitive with gravity even for luminosit

Decimate

Requirements for Theoretical Models of Outflowsr the past five days. Clearly this id an impossible task and I cannot pretend to do it justice. During the 31 years since Deutch (1956) first presented indisputable evidence for mass loss from the α Her system, the topic of mass loss has grown to be a major research area in astrophysics. The review

使顯得不重要

Esalate

integrated

Thyroxine

才能

dagger

分開

Genteel