Results 121 to 130 of about 184,376 (200)
CHANG-ES. XXX. 10 kpc Radio Lobes in the Sombrero Galaxy
We report the discovery of the 10 kpc scale radio lobes in the Sombrero galaxy (NGC 4594), using data from the Continuum Halos in Nearby Galaxies—an Expanded Very Large Array Survey project.
Yang Yang+10 more
doaj +1 more source
Possibleγ-ray Signals from Low-luminosity Active Galactic Nuclei [PDF]
Hajime Takami
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The High-mass X-Ray Binary Luminosity Functions of Dwarf Galaxies
Drawing from the Chandra archive and using a carefully selected set of nearby dwarf galaxies, we present a calibrated high-mass X-ray binary (HMXB) luminosity function in the low-mass galaxy regime and search for an already hinted at dependence on ...
Robel Geda+4 more
doaj +1 more source
The diffuse gamma-ray flux from clusters of galaxies. [PDF]
Hussain S+3 more
europepmc +1 more source
The Intrinsic Sizes of Odd Radio Circles
A new class of sources, the so-called odd radio circles (ORCs), have been discovered by recent sensitive, large-area radio continuum surveys. The distances of these sources have so far relied on photometric redshifts of optical galaxies found at the ...
David S. N. Rupke+5 more
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The cosmic ray ionization and γ-ray budgets of star-forming galaxies. [PDF]
Krumholz MR, Crocker RM, Offner SSR.
europepmc +1 more source
Circular Polarization of Simulated Images of Black Holes
Models of the resolved Event Horizon Telescope (EHT) sources Sgr A* and M87* are constrained by observations at multiple wavelengths, resolutions, polarizations, and time cadences.
Abhishek V. Joshi+4 more
doaj +1 more source
CONSTRAINING THE MAGNETIC FIELD IN THE ACCRETION FLOW OF LOW-LUMINOSITY ACTIVE GALACTIC NUCLEI
Observations show that the accretion ows in low-luminosity active galactic nuclei (LLAGNs) probably have a two-component structure with an inner hot, optically thin, advection dominated accretion ow (ADAF) and an outer truncated cool, optically thick accretion disk. As shown by Taam et al. (2012), within the framework of the disk evaporation model, the
openaire +3 more sources
We searched the Chandra and XMM archives for 900 Green Pea galaxies to identify signs of active galactic nuclei (AGN). Green peas are low-mass, emission-line galaxies that resemble high-redshift dwarf galaxies. From 29 observations, we detected X-rays in
Mainak Singha+10 more
doaj +1 more source