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Titlebook: Extragalactic Radio Sources; David S. Heeschen,Campbell M. Wade Book 1982 International Astronomical Union 1982 BL Lac object.Galaxy.Quasa

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21#
發(fā)表于 2025-3-25 05:50:32 | 只看該作者
22#
發(fā)表于 2025-3-25 08:18:01 | 只看該作者
Value Chain — das Szenario der Zukunftdio galaxies. A very small fraction of quasars do, however, show deviations from the classical double structure which are similar to the distortions observed in some low luminosity radio galaxies, e.g., bent double sources. Among radio galaxies, structural distortions seem to be associated with memb
23#
發(fā)表于 2025-3-25 15:12:40 | 只看該作者
24#
發(fā)表于 2025-3-25 17:08:51 | 只看該作者
25#
發(fā)表于 2025-3-25 22:03:17 | 只看該作者
26#
發(fā)表于 2025-3-26 01:02:25 | 只看該作者
Begriffliche und sachliche Grundlegung,d in detail (1) that the energy supply by the nuclear engine to the lobes is strongly time-dependent. Time dependent ejection from the nucleus of a parent galaxy produces low density channels which are ploughed in the background medium by the passage of intermittently ejected radio emitting plasmons
27#
發(fā)表于 2025-3-26 04:19:42 | 只看該作者
28#
發(fā)表于 2025-3-26 12:01:20 | 只看該作者
29#
發(fā)表于 2025-3-26 16:13:56 | 只看該作者
Informationstechnische Grundbildung MS-DOSt Peak to search for optical line emission associated with the jets and lobes of radio galaxies. Several sources have been found in which extended optical line emission is clearly related to the nonthermal radio emission. Some general information on these and a few other sources is summarized in Tab
30#
發(fā)表于 2025-3-26 19:13:37 | 只看該作者
https://doi.org/10.1007/978-3-322-85745-3icularly true in the case of radio galaxies where we believe that the gas is an indespensable part of the cause of nuclear activity and plays a role in the origin and the evolution of the radio galaxy phenomenon. In a few cases we are fortunate to find some of the gas to be ionized with a temperatur
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