Mass of black holes: The State of the Art
Monday, October 5th, 2009by Czerny, B. and Nikolajuk, M.
Submitted to proceedings of the Frascati Workshop 2009, Multifrequency Behaviour of High Energy Cosmic Sources, Vulcano (Italy), May 25 – 30
Editors: Pau Amaro-Seoane & Bernard Schutz
The
last GW Note is a Special Issues on eLISA/NGO
Archive for the ‘intermediate-mass black holes’ Category
Detection of IMBHs with ground-based gravitational wave observatories: A biography of a binary of black holes, from birth to death
Monday, October 5th, 2009by Amaro-Seoane, Pau and Santamaria, Lucia
Submitted to ApJ; abstract abridged, figure 1 has a lower resolution
Binaries of massive black holes in rotating clusters: Dynamics, gravitational waves, detection and the role of eccentricity
Friday, August 7th, 2009by Amaro-Seoane, Pau and Eichhorn, Christoph and Porter, Ed and Spurzem, Rainer
21 pages, 12 figs, to appear in MNRAS, abstract abridged for arxiv
Quantifying the Coexistence of Massive Black Holes and Dense Nuclear Star Clusters
Friday, July 31st, 2009Ultra-high precision cosmology from gravitational waves
Saturday, July 4th, 2009Shrinking the Braneworld: Black Hole in a Globular Cluster
Wednesday, July 1st, 2009by Gnedin, Oleg Y. and Maccarone, Thomas J. and Psaltis, Dimitrios and Zepf, Stephen E.
Density and kinematic cusps in M54 at the heart of the Sagittarius dwarf galaxy: evidence for a 10^4 M_sun Black Hole?
Tuesday, June 30th, 2009by Ibata, R. and Bellazzini, M. and Chapman, S. C. and Dalessandro, E. and Ferraro, F. R. and Irwin, M. and Lanzoni, B. and Lewis, G. F. and Mackey, A. D. and Miocchi, P. and Varghese, A.
Accepted for publication by The Astrophysical Journal (Letters). Latex. 5 pages, 4 color figures, 2 with reduced resolution, one in greyscale. A full-resolution color version of the paper can be retrieved from http://www.bo.astro.it/SGR/Sgr_BH.pdf
On the dissolution of star clusters in the Galactic centre. I. Circular orbits
Thursday, June 25th, 2009by Ernst, Andreas and Just, Andreas and Spurzem, Rainer
18 pages, 20 figures; accepted by MNRAS