activity
20062012
most citedSubmillimeter Line Emission from LMC N159W: a Dense, Clumpy PDR in a Low Metallicity Environment

36 citations · 133 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2012★ 10 cited

A mapping study of L1174 with 13CO J=2-1 and 12CO J=3-2: star formation triggered by a Herbig Ae/Be star

J. H. Yuan, Y. Wu, J. Z. Li +2

We have carried out a comprehensive study of the molecular conditions and star-forming activities in dark cloud L1174 with multi-wavelength data. Mapping observations of L1174 in $…

astro-ph.GA2010★ 14 cited

Photon Dominated Regions in NGC 3603

M. Röllig, C. Kramer, C. Rajbahak +32

Aims: We aim at deriving the excitation conditions of the interstellar gas as well as the local FUV intensities in the molecular cloud surrounding NGC 3603 to get a coherent pictur…

astro-ph2008★ 36 cited

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…

astro-ph2007★ 31 cited

12CO 4-3 and [CI] 1-0 at the centers of NGC 4945 and Circinus

M. Hitschfeld, M. Aravena, C. Kramer +30

Studying molecular gas in the central regions of the star burst galaxies NGC4945 and Circinus enables us to characterize the physical conditions and compare them to previous local…

astro-ph2007★ 34 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…

astro-ph2007★ 8 cited

Observations of V838 Mon in the CO rotational lines

T. Kaminski, M. Miller, R. Tylenda

We investigate the structure of a field around the position of V838 Mon as seen in the lowest CO rotational transitions. We also measure and analyse emission in the same lines at t…