activity
19952023
most citedThe Nuclear Spectroscopic Telescope Array (NuSTAR) Mission

2.3k citations · 41.1k across the 542 of their papers we have counts for

collaborators
Showing 2014 · astro-ph.GAShow all

7 papers · 2 filters

astro-ph.GA2014

X-ray Properties of Hard X-ray Selected AGN

Andrew C. Liebmann, Andrew C. Fabian, Sachiko Tsuruta

Using the latest 70 month Swift-BAT catalog we examined hard X-ray selected Seyfert I galaxies which are relatively little known and little studied, and yet potentially promising t…

astro-ph.GA2014★ 22 cited

A deep Chandra observation of the hot gaseous halo around a rare, extremely massive and relativistic jet launching spiral galaxy

S. A. Walker, J. Bagchi, A. C. Fabian

We present a deep Chandra observation of the extremely massive spiral galaxy 2MASX J23453268-0449256, the first X-ray observation of this very rare system which features the larges…

astro-ph.GA2014★ 16 cited

Implications of Coronal Line Emission in NGC 4696

M. Chatzikos, R. J. R. Williams, G. J. Ferland +7

We announce a new facility in the spectral code CLOUDY that enables tracking the evolution of a cooling parcel of gas with time. For gas cooling from temperatures relevant to galax…

astro-ph.GA2014★ 23 cited

Radio-mode feedback in local AGNs: dependence on the central black hole parameters

W. Ishibashi, M. W. Auger, D. Zhang +1

Radio mode feedback, in which most of the energy of an active galactic nucleus (AGN) is released in a kinetic form via radio-emitting jets, is thought to play an important role in…

astro-ph.GA2014★ 65 cited

Filamentary Star Formation in NGC 1275

R. E. A Canning, J. E. Ryon, J. S. Gallagher +8

We examine the star formation in the outer halo of NGC~1275, the central galaxy in the Perseus cluster (Abell 426), using far ultraviolet and optical images obtained with the Hubbl…

astro-ph.GA2014★ 181 cited

Dynamics of Dusty Radiation Pressure Driven Shells and Clouds: Fast Outflows from Galaxies, Star Clusters, Massive Stars, and AGN

Todd A. Thompson, Andrew C. Fabian, Eliot Quataert +1

It is typically assumed that radiation pressure driven winds are accelerated to an asymptotic velocity of V ~ v_esc, where v_esc is the escape velocity from the central source. We…