activity
20062016
most citedA Molecular Star Formation Law in the Atomic Gas Dominated Regime in Nearby Galaxies

555 citations · 3k across the 31 of their papers we have counts for

collaborators

32 papers

astro-ph.GA2016★ 168 cited

The Radio Spectral Energy Distribution and Star Formation Rate Calibration in Galaxies

F. S. Tabatabaei, E. Schinnerer, M. Krause +17

We study the spectral energy distribution (SED) of the radio continuum emission from the KINGFISH sample of nearby galaxies to understand the energetics and origin of this emission…

astro-ph.GA2015★ 46 cited

Gravitational torques imply molecular gas inflow towards the nucleus of M51

M. Querejeta, S. Meidt, E. Schinnerer +10

The transport of gas towards the centre of galaxies is critical for black hole feeding and, indirectly, it can control active galactic nucleus (AGN) feedback. We have quantified th…

astro-ph.GA2015

A High Resolution Wide-Field Radio Survey of M51

Hayden Rampadarath, John S. Morgan, Roberto Soria +4

We present the highest resolution, wide-field radio survey of a nearby face-on star-forming galaxy to date. The multi-phase centre technique is used to survey the entire disk of M5…

astro-ph.GA2015★ 93 cited

Short GMC lifetimes: an observational estimate with the PdBI Arcsecond Whirlpool Survey (PAWS)

Sharon E. Meidt, Annie Hughes, Clare L. Dobbs +10

We describe and execute a novel approach to observationally estimate the lifetimes of giant molecular clouds (GMCs). We focus on the cloud population between the two main spiral ar…

astro-ph.GA2014★ 22 cited

Revised spectroscopic parameters of SH from ALMA and IRAM 30 m observations

Holger S. P. Müller, Javier R. Goicoechea, José Cernicharo +6

Hydrides represent the first steps of interstellar chemistry. Sulfanylium (SH), in particular, is a key tracer of energetic processes. We used ALMA and the IRAM 30 m telescope…

astro-ph.GA2014★ 153 cited

Fueling AGN II: Spatially Resolved Molecular Inflows and Outflows

R. I. Davies, W. Maciejewski, E. K. S. Hicks +11

We analyse the 2-dimensional distribution and kinematics of the stars as well as molecular and ionised gas in the central few hundred parsecs of 5 active and 5 matched inactive gal…