67 citations · 302 across the 7 of their papers we have counts for
7 papers
Molecular line mapping of the giant molecular cloud associated with RCW 106 - III. Multi-molecular line mapping
N. Lo, M. R. Cunningham, P. A. Jones +10
We present multi-molecular line maps obtained with the Mopra Telescope towards the southern giant molecular cloud (GMC) complex G333, associated with the HII region RCW 106. We hav…
Optimization of mapping modes for heterodyne instruments
V. Ossenkopf
Astronomic line mapping with single-pixel instruments is usually performed in an on-the-fly (OTF) or a raster-mapping mode depending on the capabilities of the telescope and the in…
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,…
Submillimeter Line Emission from LMC N159W: a Dense, Clumpy PDR in a Low Metallicity Environment
J. L. Pineda, N. Mizuno, J. Stutzki +30
Star formation at earlier cosmological times takes place in an interstellar medium with low metallicity. The Large Magellanic Cloud (LMC) is ideally suited to study star formation…