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19962019
most citedMolecular line emission in NGC1068 imaged with ALMA. I An AGN-driven outflow in the dense molecular gas

476 citations · 10.1k across the 164 of their papers we have counts for

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Showing 2012Show all

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astro-ph.CO2012★ 107 cited

The SCUBA-2 Cosmology Legacy Survey: blank-field number counts of 450um-selected galaxies and their contribution to the cosmic infrared background

J. E. Geach, E. L. Chapin, K. E. K. Coppin +50

The first deep blank-field 450um map (1-sigma~1.3mJy) from the SCUBA-2 Cosmology Legacy Survey (S2CLS), conducted with the James Clerk Maxwell Telescope (JCMT) is presented. Our ma…

astro-ph.CO2012★ 149 cited

Evidence for CO shock excitation in NGC 6240 from Herschel SPIRE spectroscopy

R. Meijerink, L. E. Kristensen, A. Weiss +28

We present Herschel SPIRE FTS spectroscopy of the nearby luminous infrared galaxy NGC 6240. In total 20 lines are detected, including CO J=4-3 through J=13-12, 6 H2O rotational lin…

astro-ph.GA2012★ 44 cited

Hydrogenation of PAH cations: a first step towards H2 formation

L. Boschman, G. Reitsma, S. Cazaux +4

Molecular hydrogen is the most abundant molecule in the universe. A large fraction of H2 forms by association of hydrogen atoms adsorbed on polycyclic aromatic hydrocarbons (PAHs),…

astro-ph.SR2012★ 41 cited

FUV and X-ray irradiated protoplanetary disks: a grid of models II - Gas diagnostic line emission

Giambattista Aresu, Rowin Meijerink, Inga Kamp +3

Most of the mass in protoplanetary disks is in the form of gas. The study of the gas and its diagnostics is of fundamental importance in order to achieve a detailed description of…

gr-qc2012★ 2 cited

A topological extension of GR: Black holes induce dark energy

Marco Spaans

A topological extension of general relativity is presented. The superposition principle of quantum mechanics, as formulated by the Feynman path integral, is taken as a starting poi…

astro-ph.SR2012★ 49 cited

FUV and X-ray irradiated protoplanetary disks: a grid of models I. The disk structure

R. Meijerink, G. Aresu, I. Kamp +3

Context. Planets are thought to eventually form from the mostly gaseous (~99% of the mass) disks around young stars. The density structure and chemical composition of protoplanetar…