activity
20022009
most citedA complete 12CO 2-1 map of M51 with HERA: I. Radial averages of CO, HI, and radio continuum

143 citations · 398 across the 10 of their papers we have counts for

collaborators

14 papers

astro-ph.SR200967 cited

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…

astro-ph.GA200937 cited

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…

astro-ph200816 cited

The Photon Dominated Region in the IC 348 molecular cloud

K. Sun, V. Ossenkopf, C. Kramer +4

In this paper we discuss the physical conditions of clumpy nature in the IC 348 molecular cloud. We combine new observations of fully sampled maps in [C I] at 492 GHz and 12CO 4--3…

astro-ph200856 cited

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…

astro-ph200822 cited

Long-term observations of Uranus and Neptune at 90 GHz with the IRAM 30m telescope - (1985 -- 2005)

C. Kramer, R. Moreno, A. Greve

The planets Uranus and Neptune with small apparent diameters are primary calibration standards. We investigate their variability at ~90 GHz using archived data taken at the IRAM 30…

astro-ph200734 cited

Clumpy photon-dominated regions in Carina. I. [CI] and mid-J CO lines in two 4'x4' fields

C. Kramer, M. Cubick, M. Roellig +31

The Carina region is an excellent astrophysical laboratory for studying the feedback mechanisms of newly born, very massive stars within their natal giant molecular clouds (GMCs) a…