activity
20122022
most citedX-ray Signatures of Black Hole Feedback: Hot Galactic Atmospheres in IllustrisTNG and X-ray Observations

73 citations · 259 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2022

Relationships Between Stellar Velocity Dispersion and the Atmospheres of Early-Type Galaxies

R. L. S. Frisbie, M. Donahue, G. M. Voit +3

The Voit et al. (2020) black hole feedback valve model predicts relationships between stellar velocity dispersion and atmospheric structure among massive early-type galaxies. In th…

astro-ph.HE2021★ 27 cited

VLA Radio Study of a Sample of Nearby X-ray and Optically Bright Early-Type Galaxies

Romana Grossová, Norbert Werner, Francesco Massaro +9

Many massive early-type galaxies host central radio sources and hot X-ray atmospheres indicating the presence of radio-mechanical active galactic nucleus (AGN) feedback. The duty c…

astro-ph.GA2020★ 8 cited

Properties of the Hot Ambient Medium of Early-type Galaxies Hosting Powerful Radio Sources

Rachel L. S. Frisbie, Megan Donahue, G. Mark Voit +6

We present an archival analysis of Chandra X-ray observations for twelve nearby early-type galaxies hosting radio sources with radio power at 1.4…

astro-ph.HE2019★ 16 cited

How do atomic code uncertainties affect abundance measurements in the intracluster medium?

F. Mernier, N. Werner, K. Lakhchaura +6

Accurate chemical abundance measurements of X-ray emitting atmospheres pervading massive galaxies, galaxy groups, and clusters provide essential information on the star formation a…

astro-ph.GA2019★ 73 cited

X-ray Signatures of Black Hole Feedback: Hot Galactic Atmospheres in IllustrisTNG and X-ray Observations

Nhut Truong, Annalisa Pillepich, Norbert Werner +6

Hot gaseous atmospheres that permeate galaxies and extend far beyond their stellar distribution, where they are commonly referred to as the circumgalactic medium (CGM), imprint imp…

astro-ph.GA2019★ 31 cited

Correlations between supermassive black holes, hot atmospheres, and the total masses of early type galaxies

K. Lakhchaura, N. Truong, N. Werner

We present a study of relations between the masses of the central supermassive black holes (SMBHs) and the atmospheric gas temperatures and luminosities measured within a range of…

astro-ph.GA2019★ 21 cited

Powerful AGN jets and unbalanced cooling in the hot atmosphere of IC 4296

R. Grossová, N. Werner, K. Rajpurohit +13

We present new Karl G. Jansky Very Large Array (VLA, 1.5 GHz) radio data for the giant elliptical galaxy IC 4296, supported by archival radio, X-ray (Chandra, XMM-Newton) and optic…

astro-ph.GA2019★ 26 cited

Possible depletion of metals into dust grains in the core of the Centaurus cluster of galaxies

K. Lakhchaura, F. Mernier, N. Werner

We present azimuthally averaged metal abundance profiles from a full, comprehensive, and conservative re-analysis of the deep (800 ks total net exposure) \textit{Chandra}/ACI…

astro-ph.GA2018★ 24 cited

Cooling in the X-ray halo of the rotating, massive early-type galaxy NGC 7049

A. Juráňová, N. Werner, M. Gaspari +9

The relative importance of the physical processes shaping the thermodynamics of the hot gas permeating rotating, massive early-type galaxies is expected to be different from that i…

astro-ph.GA2016★ 15 cited

Decoding X-ray observations from centres of galaxy clusters using MCMC

Kiran Lakhchaura, Tarun Deep Saini, Prateek Sharma

We correct for the use of electron densities instead of total gas density in the pressure fits which were used to derive the local free-fall times (t) in the original pa…

astro-ph.GA2014★ 7 cited

Dynamics of ten clusters of galaxies with substructures

Kiran Lakhchaura, K. P. Singh

We present a detailed Chandra study of a sample of ten clusters of galaxies selected based on the presence of substructures in their optical images. The X-ray surface brightness ma…

astro-ph.CO2012★ 11 cited

A cluster pair : A3532 and A3530

K. Lakhchaura, K. P. Singh, D. J. Saikia +1

We present a detailed study of a close pair of clusters of galaxies, A3532 and A3530, and their environments. The \textit{Chandra} X-ray image of A3532 reveals presence of substruc…