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20012024
most citedA model for atomic and molecular interstellar gas: The Meudon PDR code

538 citations · 7.6k across the 116 of their papers we have counts for

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Showing 2016Show all

6 papers · 1 filter

astro-ph.GA2016★ 206 cited

The anatomy of the Orion B Giant Molecular Cloud: A local template for studies of nearby galaxies

Jérôme Pety, Viviana V. Guzmán, Jan H. Orkisz +11

We aim to develop the Orion B Giant Molecular Cloud (GMC) as a local template for interpreting extra-galactic molecular line observations. We use the wide-band receiver at the IRAM…

astro-ph.GA2016★ 22 cited

Radiative and mechanical feedback into the molecular gas in the Large Magellanic Cloud. I. N159W

Min-Young Lee, Suzanne Madden, Vianney Lebouteiller +25

We present Herschel SPIRE Fourier Transform Spectrometer (FTS) observations of N159W, an active star-forming region in the Large Magellanic Cloud (LMC). In our observations, a numb…

astro-ph.GA2016★ 18 cited

Star Formation and Feedback: A Molecular Outflow-Prestellar Core Interaction in L1689N

D. C. Lis, H. A. Wootten, M. Gerin +5

We present Herschel, ALMA Compact Array (ACA), and Caltech Submillimeter Observatory (CSO) observations of the prestellar core in L1689N, which has been suggested to be interacting…

astro-ph.GA2016★ 56 cited

A milestone toward understanding PDR properties in the extreme environment of LMC-30Dor

M. Chevance, S. C. Madden, V. Lebouteiller +11

More complete knowledge of galaxy evolution requires understanding the process of star formation and interaction between the interstellar radiation field and the interstellar mediu…

astro-ph.GA2016★ 24 cited

Collisional excitation of doubly and triply deuterated ammonia NDH and ND by H

F. Daniel, C. Rist, A. Faure +6

The availability of collisional rate coefficients is a prerequisite for an accurate interpretation of astrophysical observations, since the observed media often harbour densities w…

astro-ph.GA2016★ 19 cited

The NHD hyperfine structure revealed by astrophysical observations

F. Daniel, L. H. Coudert, A. Punanova +8

The 1-1 lines of ortho and para--NHD (o/p-NHD), respectively at 86 and 110 GHz, are commonly observed to provide constraints on the deuterium fractionation in…