activity
19982015
most citedBlack hole accretion and star formation as drivers of gas excitation and chemistry in Mrk231

315 citations · 883 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2015★ 44 cited

The JCMT Nearby Galaxies Legacy Survey X. Environmental Effects on the Molecular Gas and Star Formation Properties of Spiral Galaxies

Angus Mok, C. D. Wilson, J. Golding +9

We present a study of the molecular gas properties in a sample of 98 HI - flux selected spiral galaxies within Mpc, using the CO line observed with the James Clerk…

astro-ph.GA2014★ 104 cited

The nature of the low-frequency emission of M51: First observations of a nearby galaxy with LOFAR

D. D. Mulcahy, A. Horneffer, R. Beck +25

The grand-design spiral galaxy M51 was observed with the LOFAR High Frequency Antennas (HBA) and imaged in total intensity and polarisation. This observation covered the frequencie…

astro-ph.CO2010★ 22 cited

Excitation of the molecular gas in the nuclear region of M82

A. F. Loenen, P. P. van der Werf, R. Güsten +23

We present high resolution HIFI spectroscopy of the nucleus of the archetypical starburst galaxy M82. Six 12CO lines, 2 13CO lines and 4 fine-structure lines are detected. Besides…

astro-ph.CO2010★ 40 cited

Cool gas and dust in M33: Results from the Herschel M33 extended survey (HERM33ES)

J. Braine, P. Gratier, C. Kramer +23

We present an analysis of the first space-based far-IR-submm observations of M 33, which measure the emission from the cool dust and resolve the giant molecular cloud complexes. Wi…

astro-ph.GA2010★ 315 cited

Black hole accretion and star formation as drivers of gas excitation and chemistry in Mrk231

P. P. Van der Werf, K. G. Isaak, R. Meijerink +34

We present a full high resolution SPIRE FTS spectrum of the nearby ultraluminous infrared galaxy Mrk231. In total 25 lines are detected, including CO J=5-4 through J=13-12, 7 rotat…

astro-ph2008★ 46 cited

The Dust-to-Gas Ratio in the Small Magellanic Cloud Tail

K. D. Gordon, C. Bot, E. Muller +21

The Tail region of the Small Magellanic Cloud (SMC) was imaged using the MIPS instrument on the Spitzer Space Telescope as part of the SAGE-SMC Spitzer Legacy. Diffuse infrared emi…