activity
20072025
most citedDetection of OH and HO towards Orion~KL

48 citations · 292 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2025★ 3 cited

The Diamond Ring in Cygnus X: Advanced stage of an expanding bubble of ionised carbon

Simon M. Dannhauer, Sebastian Vider, Nicola Schneider +18

The "Diamond Ring" in Cygnus X, southwest of the DR21 ridge, is a nearly circular structure of 6 pc in diameter, prominent in FIR emission and enclosed by clumpy molecular cl…

astro-ph.GA2024

Bright-rimmed clouds in IC 1396 I. Dynamics

Yoko Okada, Slawa Kabanovic, Rolf Güsten +14

We investigate the dynamical and physical structures of bright-rimmed clouds (BRCs) in a nearby HII region. We focused on carbon- and oxygen-bearing species that trace photon-domin…

astro-ph.GA2023★ 13 cited

SOFIA FEEDBACK Survey: The Pillars of Creation in [C II] and Molecular Lines

Ramsey L. Karim, Marc W. Pound, Alexander G. G. M. Tielens +11

We investigate the physical structure and conditions of photodissociation regions (PDRs) and molecular gas within the Pillars of Creation in the Eagle Nebula using SOFIA FEEDBACK o…

physics.ins-det2014★ 1 cited

Heat transfer coefficient saturation in superconducting Nb tunnel junctions contacted to a NbTiN circuit and an Au energy relaxation layer

Stefan Selig, Marc Peter Westig, Karl Jacobs +2

In this paper we present the experimental realization of a Nb tunnel junction connected to a high-gap superconducting NbTiN embedding circuit. We investigate relaxation of nonequil…

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-ph.GA2010★ 48 cited

Detection of OH and HO towards Orion~KL

H. Gupta, P. Rimmer, J. C. Pearson +76

We report observations of the reactive molecular ions OH, HO, and HO towards Orion KL with Herschel/HIFI. All three fine-structure transitions of OH…