217 citations · 995 across the 22 of their papers we have counts for
5 papers · 1 filter
The width of Herschel filaments varies with distance
G. V. Panopoulou, S. E. Clark, A. Hacar +5
Context: Filamentary structures in nearby molecular clouds have been found to exhibit a characteristic width of 0.1 pc, as observed in dust emission. Understanding the origin of th…
The "Maggie" filament: Physical properties of a giant atomic cloud
J. Syed, J. D. Soler, H. Beuther +19
The atomic phase of the interstellar medium plays a key role in the formation process of molecular clouds. Due to the line-of-sight confusion in the Galactic plane that is associat…
Could Segue 1 be a destroyed star cluster? - a dynamical perspective
Raul Dominguez, Michael Fellhauer, Matias Blaña +5
We attempt to find a progenitor for the ultra-faint object Segue 1 under the assumption that it formed as a dark matter free star cluster in the past. We look for orbits, using the…
Fragmentation and dynamical collapse of the starless high-mass star-forming region IRDC18310-4
H. Beuther, H. Linz, J. Tackenberg +9
Aims: We study the fragmentation and dynamical properties of a massive starless gas clump at the onset of high-mass star formation. Methods: Based on Herschel continuum data we ide…
Popping star clusters as building blocks of the Milky Way Thick Disc
P. Assmann, M. Fellhauer, P. Kroupa +2
It is widely believed that star clusters form with low star formation efficiencies. With the onset of stellar winds by massive stars or finally when the first super nova blows off,…