activity
20082015
most citedGiant Molecular Filaments in the Milky Way

155 citations · 224 across the 3 of their papers we have counts for

collaborators

14 papers

astro-ph.SR2015★ 13 cited

Kinematic and Thermal Structure at the onset of high-mass star formation

S. Bihr, H. Beuther, H. Linz +6

We want to understand the kinematic and thermal properties of young massive gas clumps prior to and at the earliest evolutionary stages of high-mass star formation. Do we find sign…

astro-ph.GA2014★ 155 cited

Giant Molecular Filaments in the Milky Way

Sarah E. Ragan, Thomas Henning, Jochen Tackenberg +4

Throughout the Milky Way, molecular clouds typically appear filamentary, and mounting evidence indicates that this morphology plays an important role in star formation. What is not…

astro-ph.GA2014★ 56 cited

Kinematic structure of massive star-forming regions - I. Accretion along filaments

J. Tackenberg, H. Beuther, Th. Henning +8

The mid- and far-infrared view on high-mass star formation, in particular with the results from the Herschel space observatory, has shed light on many aspects of massive star forma…

astro-ph.GA2013

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…

astro-ph.SR2013

The earliest phases of star formation - A Herschel key project. The thermal structure of low-mass molecular cloud cores

R. Launhardt, A. M. Stutz, A. Schmiedeke +19

The temperature and density structure of molecular cloud cores are the most important physical quantities that determine the course of the protostellar collapse and the properties…

astro-ph.SR2013

G048.66-0.29: Physical State of an Isolated Site of Massive Star Formation

Jan Pitann, Hendrik Linz, Sarah Ragan +9

We present continuum observations of the infrared dark cloud (IRDC) G48.66-0.22 (G48) obtained with Herschel, Spitzer, and APEX, in addition to several molecular line observations.…