159 citations · 440 across the 7 of their papers we have counts for
7 papers
A complete 12CO 2--1 map of M51 with HERA: II. Total gas surface densities and gravitational stability
M. Hitschfeld, C. Kramer, K. F. Schuster +2
To date the onset of large-scale star formation in galaxies and its link to gravitational stability of the galactic disk have not been fully understood. The nearby face-on spiral g…
First 450-micron dust continuum mapping of the massive star-forming region NGC 3576 with the P-ArTeMiS bolometer camera
P. André, V. Minier, P. Gallais +20
Context: The earliest phases of massive star formation are currently much debated. Aims. In an effort to make progress, we took a census of Class0-like protostellar dense cores in…
The N2D+/N2H+ ratio as an evolutionary tracer of Class 0 protostars
M. Emprechtinger, P. Caselli, N. H. Volgenau +2
Deuterated ions are abundant in cold (T=10 K), dense (n=10^5 cm^-3) regions, in which CO is frozen out onto dust grains. In such environments, the deuterium fractionation of such i…
A clumpy-cloud PDR model of the global far-infrared line emission of the Milky Way
M. Cubick, J. Stutzki, V. Ossenkopf +2
The fractal structure of the interstellar medium suggests that the interaction of UV radiation with the ISM as described in the context of photon-dominated regions (PDR) dominates…
Structure analysis of interstellar clouds: II. Applying the Delta-variance method to interstellar turbulence
V. Ossenkopf, M. Krips, J. Stutzki
The Delta-variance analysis is an efficient tool for measuring the structural scaling behaviour of interstellar turbulence in astronomical maps. In paper I we proposed essential im…
Structure analysis of interstellar clouds: I. Improving the Delta-variance method
V. Ossenkopf, M. Krips, J. Stutzki
The Delta-variance analysis, has proven to be an efficient and accurate method of characterising the power spectrum of interstellar turbulence. The implementation presently in use,…