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Report by the ESA-ESO Working Group on "The Herschel-ALMA Synergies"
T. L. Wilson, D. Elbaz, eds
The Herschel Satellite and the Atacama Large Millimeter Array (ALMA) are two very large sub-mm and far infrared (FIR) astronomy projects that are expected to come into operation in…
Run-away formation of intermediate-mass black holes in dense star clusters
Marc Freitag, M. Atakan Gürkan, Frederic A. Rasio
We consider spherical stellar clusters with a broad mass function and a relaxation time short enough so that the segregation of massive stars toward the centre occurs before they h…
Dynamical Evolution of Globular Clusters in the Magellanic Clouds and Other Local Systems
A. D. Mackey, G. F. Gilmore
Observations of rich LMC and SMC clusters reveal an increasing spread in core radius with age. This trend likely represents real physical evolution in these systems. Old Magellanic…
Palomar 5 and its tidal tails: New observational results
M. Odenkirchen, E. K. Grebel, W. Dehnen +4
Sloan Digital Sky Survey data for the field of the globular cluster Pal 5 reveal the existence of a long massive stream of tidal debris spanning an arc of 10 degrees on the sky. Pa…
On the Oosterhoff Classification of the Unusual, Metal-Rich Globular Clusters NGC 6388 and NGC 6441
M. Catelan, A. V. Sweigart, B. J. Pritzl +1
We discuss the Oosterhoff classification of the unusual, metal-rich globular clusters NGC 6388 and NGC 6441, on the basis of new evolutionary models computed for a range of metalli…
HI in Early-Type Galaxies
T. Oosterloo, R. Morganti, E. M. Sadler
We briefly discuss the main differences between the HI properties of luminous and low-luminosity early-type galaxies. In luminous early-type galaxies the HI is often irregularly di…