activity
20062017
most citedWater in Star-Forming Regions with the Herschel Space Observatory (WISH): Overview of key program and first results

262 citations · 3.1k across the 53 of their papers we have counts for

collaborators

53 papers

physics.chem-ph2017★ 35 cited

Collisional excitation of NH3 by atomic and molecular hydrogen

N. Bouhafs, C. Rist, F. Daniel +4

We report extensive theoretical calculations on the rotation-inversion excitation of interstellar ammonia (NH3) due to collisions with atomic and molecular hydrogen (both para- and…

astro-ph.GA2016★ 53 cited

Deuteration of ammonia in the starless core Ophiuchus/H-MM1

Jorma Harju, Fabien Daniel, Olli Sipilä +13

Ammonia and its deuterated isotopologues probe physical conditions in dense molecular cloud cores. With the aim of testing the current understanding of the spin-state chemistry of…

astro-ph.GA2016★ 28 cited

NH and NNH towards the prestellar core 16293E in L1689N

F. Daniel, A. Faure, L. Pagani +6

Understanding the processes that could lead to enrichment of molecules in N atoms is of particular interest in order to shed light on the relatively large variations observe…

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…

astro-ph.GA2015★ 23 cited

Stratified NH and ND emission in the prestellar core 16293E in L1689N

A. Bacmann, F. Daniel, P. Caselli +6

High degrees of deuterium fractionation are commonly found in cold prestellar cores and in the envelopes around young protostars. As it brings strong constraints to chemical models…