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Titlebook: Quasar Hosts; Proceedings of the E David L. Clements,Ismael Pérez-Fournon Conference proceedings 1997 Springer-Verlag Berlin Heidelberg 199

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31#
發(fā)表于 2025-3-27 00:46:47 | 只看該作者
32#
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33#
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34#
發(fā)表于 2025-3-27 10:31:56 | 只看該作者
Resolution of High Redshift QSO Hostsopulations. Improved and quantitative data require a combination of good signal and high resolution. Existing data are discussed and the initial results of adaptive optics imaging with CFHT are presented.
35#
發(fā)表于 2025-3-27 14:54:47 | 只看該作者
36#
發(fā)表于 2025-3-27 21:05:21 | 只看該作者
Adaptive Optics Observations of Quasar Hostsquasar hosts in particular. It will allow ground-based studies at a similar spatial resolution to those currently only possible from space. The relative flexibility of observing from the ground, both in terms of available instruments and speed between applying and observing means that such technique
37#
發(fā)表于 2025-3-27 22:09:08 | 只看該作者
38#
發(fā)表于 2025-3-28 06:03:53 | 只看該作者
39#
發(fā)表于 2025-3-28 06:35:20 | 只看該作者
The Unified Schemes and Radio Polarization Studiesr-luminosity FRI sources are believed to be the parent or misaligned population of the BL Lac objects (Barthel 1989; Antonucci 1993; Urry and Padovani 1995). In this paper we discuss some of the polarization studies which might be relevant for testing or constraing the unified schemes.
40#
發(fā)表于 2025-3-28 12:31:00 | 只看該作者
Quasar Host Luminosities and the Evolutionary Unified Schemelore the behavior of the . separately for quasars and radio galaxies, I present here the distributions of two orientation indicators, namely the jet asymmetry (in the radio band) .and the apparent transverse velocity .. = . sin ./(1 ? β cos .). Results are presented for the 2nd and 3rd of the three
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