Results 131 to 140 of about 1,242,014 (263)
Relativistic superluminal radio jets in microquasars in our galaxy [PDF]
PoSMQW6:101,2006, 2006 We discuss the origin of superluminal radio jets in Black hole X-ray binaries with relativistic radio jets in our Galaxy popularly known as microquasars. We classify the relativistic superluminal jet according to the radio emission in black hole X-ray binaries (transient or persistent) rather than the mass of the companion.
arxiv
Monitoring of multi-frequency polarization of gamma-ray bright AGNs
EPJ Web of Conferences, 2013 We started two observing programs with the Korean VLBI Network (KVN) monitoring changes in the flux density and polarization of relativistic jets in gamma-ray bright AGNs simultaneously at 22, 43, 86, 129 GHz.
Lee Sang-Sung +7 more
doaj +1 more source
The jet-disk symbiosis. II. Interpreting the Radio/UV correlations in quasars [PDF]
Astron.Astrophys.298:375,1995, 1994 We investigate the correlation between the accretion disk (UV) luminosity and the radio core emission of a quasar sample. In a radio/$L_{\rm disk}$ plot we find the quasars to be separated into four classes: core dominated quasars (CDQ), lobe dominated quasars (LDQ), radio-intermediate quasars (RIQ) and radio weak quasars.
arxiv
Steady jets and transient jets: observational characteristics and models [PDF]
arXiv, 2010 Two types of radio emission are observed from X-ray binaries with jets. They have completely different characteristics and are associated with different kinds of ejections. One kind of emission has a flat or inverted spectrum indicating optically thick self-absorbed synchrotron emission; the second kind of emission corresponds to an optically thin ...
arxiv
The Astrophysical JournalWe present James Webb Space Telescope MIRI data of the inner ∼3 × 2 kpc ^2 of the galaxy IC 5063, in which the jets of a supermassive black hole interact with the gaseous disk they are crossing.
Kalliopi M. Dasyra +10 more
doaj +1 more source
JWST Reveals Powerful Feedback from Radio Jets in a Massive Galaxy at z = 4.1
The Astrophysical JournalWe report observations of a powerful ionized gas outflow in the z = 4.1 luminous radio galaxy TNJ1338-1942 hosting an obscured quasar using the Near Infrared Spectrograph (NIRSpec) on board JWST.
Namrata Roy +13 more
doaj +1 more source
VLBI Analysis of a Potential High-Energy Neutrino Emitter Blazar
UniverseRecent studies suggest that high-energy neutrinos can be produced in the jets of blazars, radio-loud active galactic nuclei (AGN) with jets pointing close to the line of sight.
Janka Kőmíves +3 more
doaj +1 more source
The Astrophysical Journal Supplement SeriesBent-tail radio galaxies (BTRGs) are characterized by bent radio lobes. This unique shape is mainly caused by the movement of the galaxy within a cluster, during which the radio jets are deflected by the intracluster medium.
Baoqiang Lao +8 more
doaj +1 more source