Results 181 to 190 of about 289,816 (297)
Cosmic ray feedback in galaxies and galaxy clusters: A pedagogical introduction and a topical review of the acceleration, transport, observables, and dynamical impact of cosmic rays. [PDF]
Ruszkowski M, Pfrommer C.
europepmc +1 more source
X-ray versus optically selected active galactic nuclei: a comparative study of the luminosity functions and evolution rates [PDF]
A. Franceschini+3 more
openalex +1 more source
The Prospects Of X-Ray Polarimetry For Active Galactic Nuclei
Polarimetry at optical and other wavelength continues to play an important role in our struggle to develop (super-)unification schemes for active galactic nuclei (AGN). Therefore, radio-loud and radio-quiet AGN are important targets for the future small and medium-size X-ray polarimetry missions that are currently under phase A study at NASA and ESA ...
openaire +2 more sources
3C 264 is one of the few FRI radio galaxies with detected TeV emission. It is a low-luminosity active galactic nucleus (LLAGN) and is generally associated with a radiatively inefficient accretion flow (RIAF).
Ka-Wah Wong+6 more
doaj +1 more source
A complete X-ray sample of the high latitude sky from HEAO-1 A-2: log N lo S and luminosity functions [PDF]
An experiment was performed in which a complete X-ray survey of the 8.2 steradians of the sky at galactic latitudes where the absolute value of b is 20 deg down to a limiting sensitivity of 3.1 x ten to the minus 11th power ergs/sq cm sec in the 2-10 ...
Boldt, E. A.+6 more
core +1 more source
An X‐Ray Spectral Survey of Radio‐loud Active Galactic Nuclei withASCA [PDF]
R. M. Sambruna+2 more
openalex +1 more source
X‐Ray Lines in Active Galactic Nuclei and Photoionized Gases [PDF]
H. Netzer
openalex +1 more source
Multiwavelength Polarization Observations of Mrk 501
Mrk 501 is a prototypical high-synchrotron-peaked blazar and serves as one of the primary targets for the Imaging X-ray Polarimetry Explorer (IXPE). In this study, we report X-ray polarization measurements of Mrk 501 based on six IXPE observations.
Xin-Ke Hu+20 more
doaj +1 more source