activity
20142025
most citedThe Effects of Consistent Chemical Kinetics Calculations on the Pressure-Temperature Profiles and Emission Spectra of Hot Jupiters

170 citations · 1k across the 24 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

5 papers · 1 filter

astro-ph.GA2017105 cited

Turbulence and star formation efficiency in molecular clouds: solenoidal versus compressive motions in Orion B

Jan H. Orkisz, Jérôme Pety, Maryvonne Gerin +13

The nature of turbulence in molecular clouds is one of the key parameters that control star formation efficiency: compressive motions, as opposed to solenoidal motions, can trigger…

astro-ph.GA201693 cited

Feedback in Clouds II: UV Photoionisation and the first supernova in a massive cloud

Sam Geen, Patrick Hennebelle, Pascal Tremblin +1

Molecular cloud structure is regulated by stellar feedback in various forms. Two of the most important feedback processes are UV photoionisation and supernovae from massive stars.…

astro-ph.GA201560 cited

Mopra CO Observations of the Bubble HII Region RCW120

L. D. Anderson, L. Deharveng, A. Zavagno +6

We use the Mopra radio telescope to test for expansion of the molecular gas associated with the bubble HII region RCW120. A ring, or bubble, morphology is common for Galactic HII r…

astro-ph.GA201487 cited

Understanding star formation in molecular clouds II. Signatures of gravitational collapse of IRDCs

N. Schneider, T. Csengeri, R. S. Klessen +6

We analyse column density and temperature maps derived from Herschel dust continuum observations of a sample of massive infrared dark clouds (G11.11-0.12, G18.82-0.28, G28.37+0.07,…

astro-ph.GA2014125 cited

Understanding star formation in molecular clouds I. Effects of line-of-sight contamination on the column density structure

N. Schneider, V. Ossenkopf, T. Csengeri +6

Column-density maps of molecular clouds are one of the most important observables in the context of molecular cloud- and star-formation (SF) studies. With the Herschel satellite it…