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Titlebook: BL Lac Objects; Proceedings of a Wor L. Maraschi,T. Maccacaro,M. -H. Ulrich Conference proceedings 1989 Springer-Verlag Berlin Heidelberg 1

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期刊全称BL Lac Objects
期刊简称Proceedings of a Wor
影响因子2023L. Maraschi,T. Maccacaro,M. -H. Ulrich
视频video
学科分类Lecture Notes in Physics
图书封面Titlebook: BL Lac Objects; Proceedings of a Wor L. Maraschi,T. Maccacaro,M. -H. Ulrich Conference proceedings 1989 Springer-Verlag Berlin Heidelberg 1
影响因子This volume gives a comprehensible survey of BL Lac objects: contributors summarize observations on these interesting astrophysical objects and present theoretical models to explain them. Understanding these objects should help to give a better insight into the physics of black holes and relativistic plasmas. Topics addressed cover radio jets expanding at superluminal velocities, possible effects of relativistic jets on interstellar matter, the continuum emission over the whole electromagnetic system and its variability, and the impact of these observations on gravitational lensing and cosmological evolution. The book should be immensely useful for graduate students.
Pindex Conference proceedings 1989
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发表于 2025-3-21 22:33:41 | 显示全部楼层
Statistics of superluminal sources,orentz factor, the Doppler boost exponent and the . exponent, . peaks at a few degrees, well inside the angle for maximum apparent transverse velocity. Theoretical distributions of the apparent transverse velocity are sharply peaked near the maximum possible value, but the observed distribution is p
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,The host galaxy of BL Lac objects or what’s in a name?,ontains mostly medium bright radio galaxies. This analysis leads us to suggest that radio galaxies such as those of the B2 bright sample form the parent population of nearby BL Lac objects. Confirmation of this model requires the identification and observation of a larger number of nearby BL Lac obj
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A spectroscopic study of blazars at medium resolution. Observations of PKS 0521-36, PKS 0537-44 andizable sample of objects through detection of weak spectral features, either in emission or in absorption; .) monitoring intensity and profile of the broad emission fines present in selected objects, in order to investigate their correlation with continuum intensity. Preliminary results obtained on
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Anisotropic ionising continuum emission in AGNs,N. The anisotropy of the ionising continuum, evident from very extended and very narrow [OIII] line emission, appears correlated with the nuclear radio axis. Further information on anisotropy may be obtained from the detailed associations between [OIII] features and radio components observed in AGNs
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Polarization OF BL Lac objects, and Faraday rotation. Wavelength- and time-dependent polarization observations of BL Lac itself are used to investigate the polarization characteristics of one variability event without resorting to the use of adjustable fitting parameters. Simultaneous and nearly-simultaneous optical and radio pol
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