activity
20002003
most citedEvolution of the polarization of the optical afterglow of the gamma-ray burst GRB 030329

116 citations · 117 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph2003116 cited

Evolution of the polarization of the optical afterglow of the gamma-ray burst GRB 030329

J. Greiner, S. Klose, K. Reinsch +23

We report 31 polarimetric observations of the afterglow of GRB 030329 with high signal-to-noise and high sampling frequency. We establish the polarization light curve, detect susta…

astro-ph2003

The Grandeur of Massive Star Formation Revealed with ISAAC

Hendrik Linz, Bringfried Stecklum, Thomas Henning +1

We present selected results from our ongoing investigation of high-mass star-forming regions which are based on infrared observations with ESO's ISAAC camera at the 8.2-m ANTU VLT…

astro-ph20021 cited

Infrared Imaging Polarimetry of Massive Star-forming Regions

Bringfried Stecklum, Thomas Henning, Markus Feldt +2

Imaging polarimetry is a useful tool to reveal the 3D structure of dust distributions and to localize embedded young stellar objects. We present maps of the linear polarization at…

astro-ph2001

High-resolution studies of massive star-forming regions

Thomas Henning, Markus Feldt, Bringfried Stecklum

We summarize the status of our program of near-infrared adaptive optics observations of ultracompact HII regions. By means of selected results we demonstrate the usefulness of this…

astro-ph2001

The extraordinarily bright optical afterglow of GRB 991208 and its host galaxy

A. J. Castro-Tirado, V. V. Sokolov, J. Gorosabel +50

Observations of the extraordinarily bright optical afterglow (OA) of GRB 991208 started 2.1 d after the event. The flux decay constant of the OA in the R-band is -2.30 +/- 0.07 up…

astro-ph2000

Pre-main sequence binaries with aligned disks ?

Sebastian Wolf, Bringfried Stecklum, Thomas Henning

We present the results of a study performed with the goal to investigate whether low-mass pre-main sequence binary stars are formed by multiple fragmentation or via stellar capture…