activity
20022025
most citedThe SILCC (SImulating the LifeCycle of molecular Clouds) project: I. Chemical evolution of the supernova-driven ISM

367 citations · 6.4k across the 103 of their papers we have counts for

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astro-ph2008★ 103 cited

Algorithmic comparisons of decaying, isothermal, supersonic turbulence

S. Kitsionas, C. Federrath, R. Klessen +10

Contradicting results have been reported in the literature with respect to the performance of the numerical techniques employed for the study of supersonic turbulence. We aim at ch…

astro-ph2008★ 101 cited

iVINE - Ionization in the parallel tree/SPH code VINE: First results on the observed age-spread around O-stars

M. Gritschneder, T. Naab, A. Burkert +3

We present a three-dimensional, fully parallelized, efficient implementation of ionizing UV radiation for smoothed particle hydrodynamics (SPH) including self-gravity. Our method i…

astro-ph2006★ 164 cited

Supernova 2006aj and the associated X-Ray Flash 060218

J. Sollerman, A. O. Jaunsen, J. P. U. Fynbo +23

We have studied the afterglow of the gamma-ray burst (GRB) of February 18, 2006. This is a nearby long GRB, with a very low peak energy, and is therefore classified as an X-ray Fla…

astro-ph2006★ 68 cited

Crystalline silicates as a probe of disk formation history

C. P. Dullemond, D. Apai, S. Walch

We present a new perspective on the crystallinity of dust in protoplanetary disks. The dominant crystallization by thermal annealing happens in the very early phases of disk format…

astro-ph2005★ 149 cited

Constraints on the Progenitor Systems of Type Ia Supernovae

Maximilian Stritzinger, Bruno Leibundgut, Stefanie Walch +1

UVOIR bolometric light curves provide valuable insight into the nature of type Ia supernovae. We present an analysis of sixteen well-observed SNe Ia. Constraints are placed on seve…

astro-ph2002★ 153 cited

Understanding the spectra of isolated Herbig stars in the frame of a passive disk model

C. Dominik, C. P. Dullemond, L. B. F. M. Waters +1

We discuss spectral energy distributions of a sample of Herbig Ae/Be stars in the context of a passive irradiated disk model. The data have been presented earlier by Meeus et al (2…