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20002026
most citedBlack hole feedback in the luminous quasar PDS 456

277 citations · 1.6k across the 46 of their papers we have counts for

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15 papers · 1 filter

astro-ph.HE2024

X-ray properties of coronal emission in radio quiet Active Galactic Nuclei

Sibasish Laha, Claudio Ricci, John C. Mather +5

Active galactic nuclei (AGN) are powerful sources of panchromatic radiation. All AGN emit in X-rays, contributing around of the AGN bolometric luminosity. The X-ray e…

astro-ph.HE2024

Power of simultaneous X-ray and UV high-resolution spectroscopy for probing AGN outflows

Missagh Mehdipour, Laura W. Brenneman, Jon M. Miller +6

Black hole accretion in active galactic nuclei (AGN) is coupled to the evolution of their host galaxies. Outflowing winds in AGN can play an important role in this evolution throug…

astro-ph.HE2024

Overionized plasma in the supernova remnant Sagittarius A East anchored by XRISM observations

XRISM Collaboration

Sagittarius A East is a supernova remnant with a unique surrounding environment, as it is located in the immediate vicinity of the supermassive black hole at the Galactic center, S…

astro-ph.HE2024

The XRISM/Resolve view of the Fe K region of Cyg X-3

XRISM Collaboration

The X-ray binary system Cygnus X-3 (4U 2030+40, V1521 Cyg) is luminous but enigmatic owing to the high intervening absorption. High-resolution X-ray spectroscopy uniquely probes th…

astro-ph.GA2024

AGN STORM 2: X. The origin of the interband continuum delays in Mrk 817

Hagai Netzer, Michael R. Goad, Aaron J. Barth +26

The local (z=0.0315) AGN Mrk 817, was monitored over more than 500 days with space-borne and ground-based instruments as part of a large international campaign AGN STORM 2. Here, w…

astro-ph.GA2024★ 1 cited

A dichotomy in the 1-24 GHz parsec-scale radio spectra of radio-quiet quasars

Sina Chen, Ari Laor, Ehud Behar +3

We present the pc-scale radio spectra of a representative sample of 13 Palomar-Green radio-quiet quasars, based on our new Very Long Baseline Array (VLBA) observations at 8.4 and 2…