activity
20032007
most cited2D velocity fields of simulated interacting disc galaxies

50 citations · 94 across the 4 of their papers we have counts for

collaborators
Showing astro-phShow all

7 papers · 1 filter

astro-ph200750 cited

2D velocity fields of simulated interacting disc galaxies

T. Kronberger, W. Kapferer, S. Schindler +1

We investigate distortions in the velocity fields of disc galaxies and their use to reveal the dynamical state of interacting galaxies at different redshift. For that purpose, we m…

astro-ph200721 cited

Investigation of transit-selected exoplanet candidates from the MACHO survey

S. D. Huegelmeyer, S. Dreizler, D. Homeier +1

Context: Planets outside our solar system transiting their host star, i. e. those with an orbital inclination near 90 degree, are of special interest to derive physical properties…

astro-ph200623 cited

XMM-Newton observation of Mrk 110

Th. Boller, I. Balestra, W. Kollatschny

We report on the first XMM-Newton observation of the bright Narrow-Line Seyfert 1 galaxy Mrk 110. We find a narrow Fe K fluorescent line, a broad component FWHM ~ 16500 km/s of the…

astro-ph2006

Observational constraints on the evolutionary connection between PG 1159 stars and DO white dwarfs

S. D. Huegelmeyer, S. Dreizler, K. Werner +3

The Sloan Digital Sky Survey has provided spectra of a large number of new PG 1159 stars and DO white dwarfs. This increase in known hot H-deficient compact objects significantly i…

astro-ph2004

AcDc - A new code for the NLTE spectral analysis of accretion discs: application to the helium CV AM CVn

T. Nagel, S. Dreizler, T. Rauch +1

We present a recently developed code for detailed NLTE calculations of accretion disc spectra of cataclysmic variables and compact X-ray binaries. Assuming a radial structure of a…

astro-ph2004

Quantitative interpretation of the rotation curves of spiral galaxies at redshifts z~0.7 and z~1

Burkhard Fuchs, Asmus Boehm, Claus Moellenhoff +1

We present decompositions of the rotation curves of three spiral galaxies at redshifts z~0.7 and 1 into contributions by their bulges, disks, and dark halos, respectively. In order…