605 citations · 2.8k across the 100 of their papers we have counts for
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Fate of clumps in damped Ly systems
Ilian T. Iliev, Hiroyuki Hirashita, Andrea Ferrara
Recent observations have revealed that damped Ly clouds (DLAs) host star formation activity. In order to examine if such star formation activity can be triggered by ionization f…
On ion-ion correlation effects during stellar core collapse
A. Marek, H. -Th. Janka, R. Buras +2
The role of ion-ion correlations in suppressing neutrino-nucleus elastic scattering during stellar core collapse is reinvestigated, using two different equations of state. We test…
Detecting Clusters of Galaxies at High Redshift with the Spitzer Space Telescope
Gillian Wilson, Adam Muzzin, Mark Lacy +1
We present an infrared adaptation of the Cluster Red-Sequence method. We modify the two filter technique of Gladders & Yee (2000) to identify clusters based on their R-[3.6] color.…
On the mass distribution of neutron stars in HMXBs
A. van der Meer, L. Kaper, M. H. van Kerkwijk +1
We present the results of a monitoring campaign of three eclipsing high-mass X-ray binaries (HMXBs: SMC X-1, LMC X-4 and Cen X-3). High-resolution VLT/UVES spectra are used to meas…
A Galactic Plane Relative Extinction Map from 2MASS
D. Froebrich, T. P. Ray, G. C. Murphy +1
We present three 14400 square degree relative extinction maps of the Galactic Plane (|b|<20degrees) obtained from 2MASS using accumulative star counts (Wolf diagrams). This method…
Galaxy Groups at 0.3 <= z <= 0.55. II. Evolution to z ~ 0
D. J. Wilman, M. L. Balogh, R. G. Bower +7
We compare deep Magellan spectroscopy of 26 groups at 0.3 <= z <= 0.55, selected from the Canadian Network for Observational Cosmology 2 field survey (CNOC2), with a large sample o…
Galaxy Groups at 0.3 <= z <= 0.55. I. Group Properties
D. J. Wilman, M. L. Balogh, R. G. Bower +5
The evolution of galaxies in groups may have important implications for the evolution of the star formation history of the universe, since many processes which operate in groups ma…