activity
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 2015 · astro-ph.GAShow all

7 papers · 2 filters

astro-ph.GA2015★ 29 cited

How chemistry influences cloud structure, star formation, and the IMF

S. Hocuk, S. Cazaux, M. Spaans +1

In the earliest phases of star-forming clouds, stable molecular species, such as CO, are important coolants in the gas phase. Depletion of these molecules on dust surfaces affects…

astro-ph.GA2015★ 13 cited

Disentangling the excitation conditions of the dense gas in M17 SW

J. P. Pérez-Beaupuits, R. Güsten, M. Spaans +7

We probe the chemical and energetic conditions in dense gas created by radiative feedback through observations of multiple CO, HCN and HCO transitions toward the dense core of…

astro-ph.GA2015★ 65 cited

Exploring the molecular chemistry and excitation in obscured luminous infrared galaxies: An ALMA mm-wave spectral scan of NGC 4418

F. Costagliola, K. Sakamoto, S. Muller +7

We obtained an ALMA Cycle 0 spectral scan of the dusty LIRG NGC 4418, spanning a total of 70.7 GHz in bands 3, 6, and 7. We use a combined local thermal equilibrium (LTE) and non-L…

astro-ph.GA2015★ 186 cited

The SCUBA-2 Cosmology Legacy Survey: ALMA resolves the bright-end of the sub-millimeter number counts

James Simpson, Ian Smail, Mark Swinbank +20

We present high-resolution 870-um ALMA continuum maps of 30 bright sub-millimeter sources in the UKIDSS UDS field. These sources are selected from deep, 1-square degrees 850-um map…

astro-ph.GA2015★ 52 cited

H2 formation on PAHs in photodissociation regions: a high-temperature pathway to molecular hydrogen

Leon Boschman, Stéphanie Cazaux, Marco Spaans +2

Molecular hydrogen is the most abundant molecule in the Universe. It is thought that a large portion of H2 forms by association of hydrogen atoms to polycyclic aromatic hydrocarbon…

astro-ph.GA2015★ 7 cited

Probing highly obscured, self-absorbed galaxy nuclei with vibrationally excited HCN

S. Aalto, S. Martin F. Costagliola, E. Gonzalez-Alfonso +16

We present high resolution (0."4) IRAM PdBI and ALMA mm and submm observations of the (ultra) luminous infrared galaxies ((U)LIRGs) IRAS17208-0014, Arp220, IC860 and Zw049.057 that…

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…