AV-node
发表于 2025-3-28 17:14:39
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有说服力
发表于 2025-3-28 19:59:51
BLR models and the L-M relation for AGNs,r function for the NGC 4151 Hß line, are the best evidences for the existence of a thick geometry in those objects. The complications due to the non-linear response of several emission lines are also discussed, and a preliminary L-M relation is suggested.
口诀
发表于 2025-3-28 23:44:16
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Gourmet
发表于 2025-3-29 04:24:21
Meteorology of the broad line region,een the variability behaviour of an emission line and the shape of its profile. Computer simulations are presented which illustrate the evolution of the line profile in response to a ‘realistic’ continuum light curve.
不怕任性
发表于 2025-3-29 10:39:59
Variability of BL Lac objects in the radio regime,PQ - HPQ population; sources aligned to a few degrees with our line of sight. The other BL Lac population consists of much less boosted, moderately variable, nearby FR I radio galaxies beamed towards us.
ambivalence
发表于 2025-3-29 12:38:54
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Canvas
发表于 2025-3-29 18:54:59
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未开化
发表于 2025-3-29 22:17:02
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animated
发表于 2025-3-30 01:41:57
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我正派
发表于 2025-3-30 05:48:44
Conference proceedings 1991 between line and continuum variability, with observational results, methodological approaches, and theoretical models accompanying each. The final part is devoted to the important aspect of propagation-induced variability.