activity
20062009
most citedA complete 12CO 2-1 map of M51 with HERA: I. Radial averages of CO, HI, and radio continuum

143 citations · 281 across the 6 of their papers we have counts for

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astro-ph200836 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-ph200731 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-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…

astro-ph2006

A complete 12CO 2-1 map of M51 with HERA

C. Kramer, M. Hitschfeld, K. F. Schuster +2

The nearby, almost face-on, and interacting galaxy M51 offers an excellent opportunity to study the distribution of molecular gas and the mechanisms governing the star formation ra…

astro-ph2006143 cited

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

K. F. Schuster, C. Kramer, M. Hitschfeld +2

The mechanisms governing the star formation rate in spiral galaxies are not yet clear. The nearby, almost face-on, and interacting galaxy M51 offers an excellent opportunity to stu…