Titlebook: Jets from Stars and Galactic Nuclei; Proceedings of a Wor Wolfgang Kundt Conference proceedings 1996 Springer-Verlag Berlin Heidelberg 1996

insurgent

AMPLE

The jets in SS 433,llowing them out to successively larger scales over eight orders of magnitude. Recent work is emphasized in this review, and care is taken to provide up-to-date entry points into the extensive older literature on SS 433. This is an update of a similar review presented three years ago (Vermeulen 1993

exceptional

Middle-Ear

Jets in planetary nebulae,nots are seen, sometimes more extended and complicated structures. Closer analysi of the simpler cases shows that they are anomalous not only in their outflow velocity, but also in their (N) abundance. The presence of a hot star further complicates their structure. Several models for the formation o

音的强弱

Derogate

inflate

Jets and QSO spectra,s at great distances from the host galaxy. In radio-loud QSOs there are clear indications that the distribution and kinematics of emission-line gas are related to the symmetry axis of the central engine, as defined by the radio jet. These jets originate at nuclear distances <0.1 pc—similar to the hi

搬运工

安装

Black hole, jet, and disk: The universal engine, the FR I/FR II break and could be explained by a powerdependent, “closing” torus. This points towards a different type of obscuring torus in radio-loud host galaxies which might be a consequence of past mergers (e.g. by the temporary formation of a binary black-hole). Interaction of the jet with th

gentle

Jets and QSO spectra,es between the two classes, and present known dependences of spectra on radio coredominance, which we interpret as dependences on the angle of the central engine to the line-of-sight. We speculate on what some of the differences may mean.