most citedHerschel/HIFI observations of spectrally resolved methylidyne signatures toward the high-mass star-forming core NGC6334I

16 citations · 16 across the 1 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2011

Shocked water in the Cep E protostellar outflow

B. Lefloch, J. Cernicharo, S. Pacheco +1

Previous far-infrared observations at low-angular resolution have reported the presence of water associated with low-velocity outflow shocks and protostellar envelopes. The outflow…

astro-ph.GA2010

Nitrogen hydrides in the cold envelope of IRAS16293-2422

Pierre Hily-Blant, Sébastien Maret, Aurore Bacmann +4

Nitrogen is the fifth most abundant element in the Universe, yet the gas-phase chemistry of N-bearing species remains poorly understood. Nitrogen hydrides are key molecules of nitr…

astro-ph.GA2010

The methanol lines and hot core of OMC2-FIR4, an intermediate-mass protostar, with Herschel-HIFI

M. Kama, C. Dominik, S. Maret +61

In contrast with numerous studies on the physical and chemical structure of low- and high-mass protostars, much less is known about their intermediate-mass counterparts, a class of…

astro-ph.GA2010

First detection of ND in the solar-mass protostar IRAS16293-2422

A. Bacmann, E. Caux, P. Hily-Blant +64

In the past decade, much progress has been made in characterising the processes leading to the enhanced deuterium fractionation observed in the ISM and in particular in the cold, d…

astro-ph.GA2010★ 16 cited

Herschel/HIFI observations of spectrally resolved methylidyne signatures toward the high-mass star-forming core NGC6334I

M. H. D. van der Wiel, F. F. S. van der Tak, D. C. Lis +65

In contrast to extensively studied dense star-forming cores, little is known about diffuse gas surrounding star-forming regions. We study molecular gas in the high-mass star-formin…

astro-ph.SR2010

Ortho-to-para ratio of interstellar heavy water

C. Vastel, C. Ceccarelli, E. Caux +65

Despite the low elemental deuterium abundance in the Galaxy, enhanced molecular D/H ratios have been found in the environments of low-mass star forming regions, and in particular t…