Results 71 to 80 of about 282 (177)
Thickness of Nanoscale Poly(Dimethylsiloxane) Layers Determines the Motion of Sliding Water Drops
Polydimethylsiloxane brushes are extensively utilized in material applications as a hydrophobic coating due to the low liquid drop friction and high stability. However, the drop movements still vary depending on how it is prepared. In this work, the film thickness is proved to be a determinant for the water drop dynamic friction on such kind of a ...
Xiaoteng Zhou +8 more
wiley +1 more source
Optical Variability of Blazars in the Tomo-e Gozen Northern Sky Transient Survey
We studied the optical variability of 241 BL Lacertae (BL Lacs) and 83 flat-spectrum radio quasars (FSRQs) from the 4LAC catalog using data from the Tomo-e Gozen Northern Sky Transient Survey, with ∼50 epochs per blazar on average.
TianFang Zhang +16 more
doaj +1 more source
Jet collimation and acceleration in the flat spectrum radio quasar 1928+738
Using time-resolved multifrequency Very Long Baseline Array data and new KaVA (KVN and VERA Array) observations, we study the structure and kinematics of the jet of the flat spectrum radio quasar (FSRQ) 1928+738. We find two distinct jet geometries as a function of distance from the central black hole, with the inner jet having a parabolic shape ...
Kunwoo Yi +4 more
openaire +2 more sources
Probing extreme black‐hole outflows on short timescales via high spectral‐resolution x‐ray imagers
Abstract We investigate outflows and the physics of super‐Eddington versus sub‐Eddington regimes in black hole systems. Our focus is on prospective science using next‐generation high‐resolution soft x‐ray instruments. We highlight the properties of black hole ultraluminous x‐ray source (ULX) systems in particular. Owing to scale invariance in accreting
C. Pinto +9 more
wiley +1 more source
Lessons from the apparent peculiar nature of the star TYC 6544‐3483‐1
Abstract We report a radio and optical study of the star TYC 6544‐3483‐1 originally selected as a follow‐up target in the course of our efforts to cross‐identify Galactic high‐energy sources. The star by itself finally turned out to be a very ordinary main‐sequence star despite the initial expectations that apparently pointed to the contrary.
Josep Martí +5 more
wiley +1 more source
Jets, black holes and disks in blazars
The Fermi and Swift satellites, together with ground based Cherenkov telescopes, has greatly improved our knowledge of blazars, namely Flat Spectrum Radio Quasars and BL Lac objects, since all but the most powerful emit most of their electro–magnetic ...
Ghisellini Gabriele
doaj +1 more source
Cross‐Polarization Gain Calibration of Linearly Polarized VLBI Antennas by Observations of 4C 39.25
Abstract Radio telescopes with dual linearly polarized feeds regularly participate in Very Long Baseline Interferometry. One example is the VLBI Global Observing System (VGOS), which is employed for high‐precision geodesy and astrometry. In order to achieve the maximum signal‐to‐noise ratio, the visibilities of all four polarization products are ...
F. Jaron +14 more
wiley +1 more source
Flat-spectrum radio quasars (FSRQs) are among the most energetic and powerful active galactic nuclei, often exhibiting jet powers comparable to or exceeding the Eddington luminosity.
Hritwik Bora +3 more
doaj +1 more source
M_BH - sigma relation in SDSS flat-spectrum radio quasars
6 pages, 4 figures, accepted to ...
Gu, Minfeng, Chen, Zhaoyu, Cao, Xinwu
openaire +2 more sources
Active galactic nuclei (AGNs) are characterized by strong temporal flux density variability across the electromagnetic spectrum, offering insights into the complex physical processes governing accretion and plasma outflows.
Lang Cui +5 more
doaj +1 more source

