Optimum
发表于 2025-3-23 10:19:12
http://reply.papertrans.cn/17/1637/163680/163680_11.png
antecedence
发表于 2025-3-23 14:54:16
0067-0057 ame of the Scientific Committee). I attempted to focus the attention of participants on the fact that, in many instances, we tend to discuss jets in terms of simple physics, more or less as one did at the time extragalactic radio sources were discovered: for instance, we still use equipartition argu
Lipoprotein
发表于 2025-3-23 21:53:02
http://reply.papertrans.cn/17/1637/163680/163680_13.png
Lyme-disease
发表于 2025-3-23 22:40:40
http://reply.papertrans.cn/17/1637/163680/163680_14.png
seruting
发表于 2025-3-24 04:39:07
Small Scale Structure of Nonthermal Radio Sources,k radio sources (Seyfert galaxies and mildly active “normal” galaxies), 7. Concluding remarks. The tables attached include lists of objects and samples observed by VLBI (and reported about during the publication period 1981/1982) and of nearby galaxies detected with VLBI.
bromide
发表于 2025-3-24 08:47:57
Bent Jets and Tailed Radio Galaxies,axies can provide a strong constraint on the average velocity of the plasma flow -- a contraint not possible for straight jets. It is also shown that the wide-angle tailed sources must be bent by a mechanism other than dynamic pressure resulting from motion through the ICM.
集合
发表于 2025-3-24 12:01:33
http://reply.papertrans.cn/17/1637/163680/163680_17.png
转换
发表于 2025-3-24 17:07:19
Physical Properties of the Jet in NGC6251,885 MHz, and a resolution of 50″ at 1446 and 1662 MHz. The resulting maps (e.g. Figure 1) give exceptionally detailed information on the distributions of the total and polarized intensities over the jet.
Gustatory
发表于 2025-3-24 22:06:40
Jet-Like Structures in Low Frequency Variable Sources,that a large number of these sources display a jet-like structure on angular scale of milliarcseconds. Furthermore, observations on arcsecond scale show that very often the sources have large scale structures in addition to their compact core.
FLORA
发表于 2025-3-25 00:34:07
Rapid Variability of 3C273 at 300 GHz,we observed a sudden drop in flux density by 11.6 ± 2.9 Jy (spectral index assumed to be zero, and all known errors included). In an interpretation with the model of bulk relativistic motion we can combine the brightness temperature inferred with the observed superluminal motion and derive strict limits on the model parameters.