241 citations · 1.1k across the 14 of their papers we have counts for
14 papers
The evolution of temperature and density structures of OB cluster-forming molecular clumps
Yuxin Lin, Friedrich Wyrowski, Hauyu Baobab Liu +4
OB star clusters originate from parsec-scale massive molecular clumps. We aim to understand the evolution of temperature and density structures on the intermediate-scale ($\lesssim…
Cold CO gas in the envelopes of FU Orionis-type young eruptive stars
Á. Kóspál, P. Ábrahám, T. Csengeri +3
FUors are young stellar objects experiencing large optical outbursts due to highly enhanced accretion from the circumstellar disk onto the star. FUors are often surrounded by massi…
Disentangling the ISM phases of the dwarf galaxy NGC 4214 using [CII] SOFIA/GREAT observations
Katja Fahrion, Diane Cormier, Frank Bigiel +9
The [CII] 158 um fine structure line is one of the dominant cooling lines in the interstellar medium (ISM) and is an important tracer of star formation. Recent velocity-resolved st…
ATLASGAL-selected massive clumps in the inner Galaxy III. Dust Continuum Characterization of an Evolutionary Sample
C. König, J. S. Urquhart, T. Csengeri +8
The ATLASGAL survey provides an ideal basis for detailed studies of large numbers of massive star forming clumps covering the whole range of evolutionary stages. The ATLASGAL Top10…
The upGREAT 1.9 THz multi-pixel high resolution spectrometer for the SOFIA Observatory
C. Risacher, R. Guesten, J. Stutzki +19
We present a new multi-pixel high resolution (R >10^7) spectrometer for the Stratospheric Observatory for Far-Infrared Astronomy (SOFIA). The receiver uses 2 x 7-pixel subarrays in…
New debris disks in nearby young moving groups
A. Moór, Á. Kóspál, P. Ábrahám +5
A significant fraction of nearby young moving group members harbor circumstellar debris dust disks. Due to their proximity and youth, these disks are attractive targets for studyin…