125 citations · 208 across the 4 of their papers we have counts for
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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…
Detecting scattered light from low-mass molecular cores at 3.6 m - Impact of global effects on the observation of coreshine
J. Steinacker, M. Andersen, W. -F. Thi +1
Recently discovered scattered light at 3-5 m from low-mass cores (so-called "coreshine") reveals the presence of grains around 1 m, which is larger than the grains found in t…
The distribution of water in the high-mass star-forming region NGC 6334I
M. Emprechtinger, D. C. Lis, T. Bell +66
We present observations of twelve rotational transitions of H2O-16, H2O-18, and H2O-17 toward the massive star-forming region NGC 6334 I, carried out with Herschel/HIFI as part of…
Direct evidence of dust growth in L183 from MIR light scattering
J. Steinacker, L. Pagani, A. Bacmann +1
Theoretical arguments suggest that dust grains should grow in the dense cold parts of molecular clouds. Evidence of larger grains has so far been gathered in near/mid infrared exti…