430 citations · 7.5k across the 119 of their papers we have counts for
14 papers · 1 filter
Pressure profiles and mass estimates using high-resolution Sunyaev-Zel'dovich effect observations of Zwicky 3146 with MUSTANG-2
Charles E. Romero, Jonathan Sievers, Vittorio Ghirardini +12
The galaxy cluster Zwicky 3146 is a sloshing cool core cluster at that in X-ray imaging does not appear to exhibit significant pressure substructure in the intracluster m…
Exploring the multiphase medium in MKW 08: from the central active galaxy up to cluster scales
A. Tümer, F. Tombesi, H. Bourdin +3
The study of the brightest cluster galaxy (BCG) coronae embedded in noncool core (NCC) galaxy clusters is crucial to understand the BCG's role in galaxy cluster evolution as well a…
Multiphase quasar-driven outflows in PG 1114+445. I. Entrained ultra-fast outflows
Roberto Serafinelli, Francesco Tombesi, Fausto Vagnetti +3
Substantial evidence in the last few decades suggests that outflows from supermassive black holes (SMBH) may play a significant role in the evolution of galaxies.Large-scale outflo…
Spectral imaging of the thermal Sunyaev-Zel'dovich effect in X-COP galaxy clusters: method and validation
Anna Silvia Baldi, Hervé Bourdin, Pasquale Mazzotta +4
The imaging of galaxy clusters through the Sunyaev--Zel'dovich effect is a valuable tool to probe the thermal pressure of the intra-cluster gas, especially in the outermost regions…
Jet-driven galaxy-scale gas outflows in the hyper-luminous quasar 3C273
B. Husemann, V. N. Bennert, K. Jahnke +6
We present an unprecedented view on the morphology and kinematics of the extended narrow-line region (ENLR) and molecular gas around the prototypical hyper-luminous quasar 3C273 ($…
Nustar Measurement Of Coronal Temperature In Two Luminous, High Redshift Qsos
G. Lanzuisi, R. Gilli, M. Cappi +13
X-ray emission from AGN is believed to be produced via Comptonization of optical/UV seed photons emitted by the accretion disk, up-scattered by hot electrons in a corona surroundin…
The X-ray Halo Scaling Relations of Supermassive Black Holes
M. Gaspari, D. Eckert, S. Ettori +13
We carry out a comprehensive Bayesian correlation analysis between hot halos and direct masses of supermassive black holes (SMBHs), by retrieving the X-ray plasma properties (tempe…
Supermassive Black Hole Feedback
Mateusz Ruszkowski, Daisuke Nagai, Irina Zhuravleva +23
Understanding the processes that drive galaxy formation and shape the observed properties of galaxies is one of the most interesting and challenging frontier problems of modern ast…
The physics and astrophysics of X-ray outflows from Active Galactic Nuclei
Sibasish Laha, Randall Smith, Panayiotis Tzanavaris +20
The highly energetic outflows from Active Galactic Nuclei detected in X-rays are one of the most powerful mechanisms by which the central supermassive black hole (SMBH) interacts w…
Probing Macro-Scale Gas Motions and Turbulence in Diffuse Cosmic Plasmas
Esra Bulbul, Massimo Gaspari, Gabriella Alvarez +31
Clusters of galaxies, the largest collapsed structures in the Universe, are located at the intersection of extended filaments of baryons and dark matter. Cosmological accretion ont…
Galaxy Winds in the Age of Hyperdimensional Astrophysics
Grant R. Tremblay, Evan E. Schneider, Alexey Vikhlinin +9
The past decade began with the first light of ALMA and will end at the start of the new era of hyperdimensional astrophysics. Our community-wide movement toward highly multiwavelen…
On the Assembly Bias of Cool Core Clusters Traced by H Nebulae
Elinor Medezinski, Michael McDonald, Surhud More +5
Do cool-core (CC) and noncool-core (NCC) clusters live in different environments? We make novel use of H emission lines in the central galaxies of redMaPPer clusters as proxies…
Black hole mass of central galaxies and cluster mass correlation in cosmological hydro-dynamical simulations
Luigi Bassini, Elena Rasia, Stefano Borgani +8
Recently, relations connecting the SMBH mass of central galaxies and global properties of the hosting cluster, such as temperature and mass, were observed. We investigate the corre…
Constraining Gas Motions in the Intra-Cluster Medium
A. Simionescu, J. ZuHone, I. Zhuravleva +9
The detailed velocity structure of the diffuse X-ray emitting intra-cluster medium (ICM) remains one of the last missing key ingredients in understanding the microphysical properti…