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Titlebook: Astrophysical Jets; Proceedings of an In A. Ferrari,A. G. Pacholczyk Conference proceedings 1983 D. Reidel Publishing Company, Dordrecht, H

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樓主: lumbar-puncture
21#
發(fā)表于 2025-3-25 03:46:05 | 只看該作者
Astrophysical Jets: Optical Morphologies of Radio Jets and their Parent Galaxies,st in particular on the morphology of the optical jets known as yet, especially that of M87, from high-resolution observations. We also discuss the new insights that the detection of interstellar dust can bring on the jet phenomenon as related to the star and dust system of the parent galaxy.
22#
發(fā)表于 2025-3-25 09:15:55 | 只看該作者
PKS 0521-36, A BL Lac Object with an Optical and Radio Jet,not clear how all of these various features relate to one another and whether they can be unified. It is worthwhile listing them all in the hope that this might provide insight into the evolution of such an object.
23#
發(fā)表于 2025-3-25 14:27:22 | 只看該作者
24#
發(fā)表于 2025-3-25 15:54:19 | 只看該作者
25#
發(fā)表于 2025-3-25 21:35:55 | 只看該作者
Der Staat und die gelehrigen K?rper885 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.
26#
發(fā)表于 2025-3-26 02:00:57 | 只看該作者
https://doi.org/10.1007/978-3-658-22789-0that 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.
27#
發(fā)表于 2025-3-26 05:36:00 | 只看該作者
Zeichen und Diskurs bei Port-Royalwe 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.
28#
發(fā)表于 2025-3-26 09:27:03 | 只看該作者
Duns Scotus and Multidimensional Freedom,st in particular on the morphology of the optical jets known as yet, especially that of M87, from high-resolution observations. We also discuss the new insights that the detection of interstellar dust can bring on the jet phenomenon as related to the star and dust system of the parent galaxy.
29#
發(fā)表于 2025-3-26 12:52:39 | 只看該作者
https://doi.org/10.1057/9780230592322not clear how all of these various features relate to one another and whether they can be unified. It is worthwhile listing them all in the hope that this might provide insight into the evolution of such an object.
30#
發(fā)表于 2025-3-26 19:00:45 | 只看該作者
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