activity
20052026
most citedProbing the evolution of molecular cloud structure: From quiescence to birth

442 citations · 3.7k across the 60 of their papers we have counts for

collaborators
Showing 2016Show all

6 papers · 1 filter

astro-ph.GA2016★ 52 cited

The HI/OH/Recombination line survey of the inner Milky Way (THOR)

H. Beuther, S. Bihr, M. Rugel +27

Context: The past decade has witnessed a large number of Galactic plane surveys at angular resolutions below 20". However, no comparable high-resolution survey exists at long radio…

astro-ph.GA2016★ 26 cited

Earliest phases of star formation (EPoS): Dust temperature distributions in isolated starless cores

N. Lippok, R. Launhardt, Th. Henning +9

Constraining the temperature and density structure of dense molecular cloud cores is fundamental for understanding the initial conditions of star formation. We use Herschel observa…

astro-ph.GA2016★ 5 cited

Appearance of Dusty Filaments at Different Viewing Angles

R. -A. Chira, R. Siebenmorgen, Th. Henning +1

Context: In the last years, there have been many studies on the omnipresence and structures of filaments in star-forming regions, as well as their role in the process of star forma…

astro-ph.GA2016★ 69 cited

Giant molecular filaments in the Milky Way II: The fourth Galactic quadrant

J. Abreu-Vicente, S. Ragan, J. Kainulainen +3

Filamentary structures are common morphological features of the cold, molecular interstellar medium (ISM). Recent studies have discovered massive, hundred-parsec-scale filaments th…

astro-ph.GA2016★ 97 cited

Resolving the fragmentation of high line-mass filaments with ALMA: the integral shaped filament in Orion A

Jouni Kainulainen, Amelia M. Stutz, Thomas Stanke +5

We study the fragmentation of the nearest high line-mass filament, the integral shaped filament (ISF, line-mass 400 M pc) in the Orion A molecular cloud. We h…

astro-ph.GA2016★ 79 cited

VISION - Vienna survey in Orion I. VISTA Orion A Survey

Stefan Meingast, João Alves, Diego Mardones +17

Orion A hosts the nearest massive star factory, thus offering a unique opportunity to resolve the processes connected with the formation of both low- and high-mass stars. Here we p…