activity
20002015
most citedUnderstanding star formation in molecular clouds III. Probability distribution functions of molecular lines in Cygnus X

77 citations · 197 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2015★ 77 cited

Understanding star formation in molecular clouds III. Probability distribution functions of molecular lines in Cygnus X

N. Schneider, S. Bontemps, F. Motte +11

Column density (N) PDFs serve as a powerful tool to characterize the physical processes that influence the structure of molecular clouds. Star-forming clouds can best be characteri…

astro-ph.GA2010★ 16 cited

Herschel observations of deuterated water towards Sgr B2(M)

Claudia Comito, Peter Schilke, Rainer Rolffs +53

Observations of HDO are an important complement for studies of water, because they give strong constraints on the formation processes -- grain surfaces versus energetic process in…

astro-ph.GA2010★ 53 cited

Herschel observations of extra-ordinary sources: Detection of Hydrogen Fluoride in absorption towards Orion~KL

T. G. Phillips, E. A. Bergin, D. C. Lis +52

We report a detection of the fundamental rotational transition of hydrogen fluoride in absorption towards Orion KL using Herschel/HIFI. After the removal of contaminating features…

astro-ph.GA2010★ 21 cited

Herschel observations in the ultracompact HII region Mon R2: Water in dense Photon-dominated regions (PDRs)

A. Fuente, O. Berne, J. Cernicharo +42

Mon R2, at a distance of 830 pc, is the only ultracompact HII region (UC HII) where the photon-dominated region (PDR) between the ionized gas and the molecular cloud can be resolve…

astro-ph.GA2010★ 30 cited

Herschel-PACS spectroscopy of the intermediate mass protostar NGC7129 FIRS 2

M. Fich, D. Johnstone, T. A. van Kempen +58

Aims: We present preliminary results of the first Herschel spectroscopic observations of NGC7129 FIRS2, an intermediate mass star-forming region. We attempt to interpret the observ…

astro-ph2000

Turbulent Velocity Structure in Molecular Clouds

Volker Ossenkopf, Mordecai-Mark Mac Low

We compare velocity structure in the Polaris Flare molecular cloud at scales ranging from 0.015 pc to 20 pc to simulations of supersonic hydrodynamic and MHD turbulence computed wi…