Results 71 to 80 of about 217,086 (193)

Recognizing Blazars Using Radio Morphology from the VLA Sky Survey

open access: yesThe Astrophysical Journal
Blazars are radio-loud active galactic nuclei whose jets have a very small angle to our line of sight. Observationally, the radio emissions are mostly compact or compact-core with a one-sided jet.
Zhang-Liang Xie   +6 more
doaj   +1 more source

The unified model of compact radio sources [PDF]

open access: yesarXiv, 2002
We propose the unified model of compact radio sources, i.e. of pulsars, maser sources, and active galactic nuclei. The unification is based on the wavelength dependence of radio source size. It is shown that the compact sources are characterized by a maser amplification of thermal radio emission. The density, temperature, and magnetic field profiles of
arxiv  

Next‐Generation Photosensitizers: Cyanine‐Carborane Salts for Superior Photodynamic Therapy of Metastatic Cancer

open access: yesAngewandte Chemie, Volume 137, Issue 9, February 24, 2025.
We report a multifaceted assessment of novel cyanine‐carborane salts as potent photosensitizers for photodynamic therapy (PDT). These compounds exhibit efficient tumor targeting through uptake by organic anion‐transporting polypeptides (OATP). Upon near‐infrared (NIR) light irradiation, cyanine‐carborane salts generate reactive oxygen species (ROS ...
Amir Roshanzadeh   +10 more
wiley   +1 more source

VaDAR: Varstrometry for Dual AGN Using Radio Interferometry

open access: yesThe Astrophysical Journal
Binary and dual active galactic nuclei (AGNs) are an important observational tool for studying the formation and dynamical evolution of galaxies and supermassive black holes.
Emma Schwartzman   +7 more
doaj   +1 more source

Investigating the Star Formation Characteristics of Radio Active Galactic Nuclei

open access: yesThe Astrophysical Journal
The coevolution of supermassive black holes and their host galaxies represents a fundamental question in astrophysics. One approach to investigating this question involves comparing the star formation rates (SFRs) of active galactic nuclei (AGNs) with ...
Bojun Zhang   +7 more
doaj   +1 more source

The radio spectra of galactic nuclei [PDF]

open access: yesarXiv, 1997
We present a model for the inverted radio spectra of active active galactic nuclei as well as the central regions of normal galaxies. The model is based on the unified scenario for active galaxies, stating that the central engines of active galaxies consists of a supermassive black hole surrounded by an accretion disk and a radio jet.
arxiv  

Deciphering Radio Emissions from Accretion Disk Winds in Radio-quiet Active Galactic Nuclei

open access: yesThe Astrophysical Journal
Unraveling the origins of radio emissions from radio-quiet active galactic nuclei (RQ AGNs) remains a pivotal challenge in astrophysics. One potential source of this radiation is the shock interaction between AGN disk winds and the interstellar medium ...
Tomoya Yamada   +3 more
doaj   +1 more source

Galactic jet sources and the AGN connection [PDF]

open access: yesarXiv, 1995
In order to further test our hypothesis that jets and disk around compact accreting objects are symbiotic features we investigate the newly discovered superluminal galactic radio jets GRS 1915+105 and GRO J1655-40 and the two famous galactic radio jets 1E1740-2942 and SS 433 within the framework of our couple jet/disk model developed initially for ...
arxiv  

Do All the Quasars and High-excitation Radio Galaxies (HERGs) in the 3CRR Catalog Contain a Magnetically Arrested Disk (MAD)?

open access: yesThe Astrophysical Journal
Based on the magnetization, an accretion disk with a large-scale magnetic field can be separated into either standard and normal evolution or magnetically arrested disk (MAD), which are difficult to identify from observations. It is still unclear whether
Shuang-Liang Li, Wenwen Zuo, Xinwu Cao
doaj   +1 more source

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