activity
20102021
most citedWind from the black-hole accretion disk driving a molecular outflow in an active galaxy

394 citations · 1.5k across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.GA2021★ 36 cited

BASS XXIX: The near-infrared view of the BLR: the effects of obscuration in BLR characterisation

Ricci F., Treister E., Bauer F. E. +24

Virial black hole mass () determination directly involves knowing the broad line region (BLR) clouds velocity distribution, their distance from the central supermassive bla…

astro-ph.GA2015★ 179 cited

The Herschel Comprehensive (U)LIRG Emission Survey (HerCULES): CO Ladders, fine structure lines, and neutral gas cooling

M. J. F. Rosenberg, P. P. van der Werf, S. Aalto +27

(Ultra) Luminous Infrared Galaxies ((U)LIRGs) are objects characterized by their extreme infrared (8-1000 m) luminosities (L and L…

astro-ph.HE2015★ 394 cited

Wind from the black-hole accretion disk driving a molecular outflow in an active galaxy

F. Tombesi, M. Melendez, S. Veilleux +3

Powerful winds driven by active galactic nuclei (AGN) are often invoked to play a fundamental role in the evolution of both supermassive black holes (SMBHs) and their host galaxies…

astro-ph.GA2014★ 8 cited

A magnified view of star formation at redshift 0.9 from two lensed galaxies

Alice Olmstead, Jane R. Rigby, Mark Swinbank +1

We present new narrow-band H alpha imaging from the Hubble Space Telescope of two redshift 0.91 galaxies that have been lensed by foreground galaxy cluster Abell 2390. These data p…

astro-ph.GA2014★ 215 cited

ALMA Reveals the Molecular Medium Fueling the Nearest Nuclear Starburst

Adam K. Leroy, Alberto D. Bolatto, Eve C. Ostriker +11

We use ALMA to derive the mass, length, and time scales associated with the nuclear starburst in NGC 253. This region forms ~2 M_sun/yr of stars and resembles other starbursts in s…

astro-ph.GA2014★ 8 cited

Extended, Dusty Star Formation Fueled by a Residual Cooling Flow in the Cluster of Galaxies Sersic 159-03

M. McDonald, N. Werner, J. B. R. Oonk +1

While the cooling of the hot intra-cluster medium (ICM) in the cores of galaxy clusters is mostly counteracted by heating from the central active galactic nucleus (AGN), the balanc…