122 citations · 462 across the 8 of their papers we have counts for
8 papers
Evaporation and condensation of spherical interstellar clouds. Self-consistent models with saturated heat conduction and cooling
W. Vieser, G. Hensler
Shortened version: The fate of IS clouds embedded in a hot tenuous medium depends on whether the clouds suffer from evaporation or whether material condensates onto them. Analytica…
Simulations of galactic winds and starbursts in galaxy clusters
W. Kapferer, C. Ferrari, W. Domainko +7
We present an investigation of the metal enrichment of the intra-cluster medium (ICM) by galactic winds and merger-driven starbursts. We use combined N-body/hydrodynamic simulation…
Subluminous O stars from the ESO Supernova Progenitor Survey - Observation versus Theory
A. Stroeer, U. Heber, T. Lisker +2
The ESO Supernova Progenitor Survey (SPY) has identified 58 (mostly helium-rich) subluminous O stars. We use the Balmer line strength to distinguish sdO from He-sdO (no Balmer line…
Spot-like Structures of Neutron Star Surface Magnetic Fields
U. Geppert, M. Rheinhardt, J. Gil
There is growing evidence, based on both X-ray and radio observations of isolated neutron stars, that besides the large--scale (dipolar) magnetic field, which determines the pulsar…
Arakelian 564: An XMM-Newton view
C. Vignali, W. N. Brandt, Th. Boller +2
We report on two XMM-Newton observations of the bright narrow-line Seyfert 1 galaxy Ark 564 taken one year apart (2000 June and 2001 June). The 0.6-10 keV continuum is well describ…
A Homogeneous Sample of Sub-DLAs II: Statistical, Kinematic and Chemical Properties
Celine Peroux, Miroslava Dessauges-Zavadsky, Sandro D'Odorico +2
Damped Ly-alpha Systems (DLAs), with N(HI)>2*10^20 cm^{-2}, observed in quasars have allowed us to quantify the chemical content of the Universe over cosmological scales. Such stud…