activity
20072026
most citedATLASGAL --- properties of a complete sample of Galactic clumps

362 citations · 7.1k across the 137 of their papers we have counts for

collaborators
Showing 2012Show all

6 papers · 1 filter

astro-ph.GA2012★ 278 cited

ATLASGAL - Compact source catalogue: 330 < l < 21 degrees

Y. Contreras, F. Schuller, J. S. Urquhart +12

Context. The APEX Telescope Large Area Survey of the Galaxy (ATLASGAL) is the first systematic survey of the inner Galactic plane in the sub-millimetre. The observations were carri…

astro-ph.GA2012★ 42 cited

The chemistry of C3 & Carbon Chain Molecules in DR21(OH)

B. Mookerjea, G. Hassel, M. Gerin +14

(Abridged) We have observed velocity resolved spectra of four ro-vibrational far-infrared transitions of C3 between the vibrational ground state and the low-energy nu2 bending mode…

astro-ph.GA2012★ 226 cited

The spine of the swan: A Herschel study of the DR21 ridge and filaments in Cygnus X

M. Hennemann, F. Motte, N. Schneider +31

In order to characterise the cloud structures responsible for the formation of high-mass stars, we present Herschel observations of the DR21 environment. Maps of the column density…

astro-ph.GA2012★ 45 cited

Globules and pillars seen in the [CII] 158 micron line with SOFIA

N. Schneider, R. Güsten, P. Tremblin +22

Molecular globules and pillars are spectacular features, found only in the interface region between a molecular cloud and an HII-region. Impacting Far-ultraviolet (FUV) radiation c…

astro-ph.GA2012★ 358 cited

Cluster-formation in the Rosette molecular cloud at the junctions of filaments

N. Schneider, T. Csengeri, M. Hennemann +31

For many years feedback processes generated by OB-stars in molecular clouds, including expanding ionization fronts, stellar winds, or UV-radiation, have been proposed to trigger su…

astro-ph.GA2012★ 17 cited

SOFIA observations of far-infrared hydroxyl emission toward classical ultracompact HII/OH maser regions

T. Csengeri, K. M. Menten, F. Wyrowski +6

The hydroxyl radical (OH) is found in various environments within the interstellar medium (ISM) of the Milky Way and external galaxies, mostly either in diffuse interstellar clouds…