Statistics – Computation
Scientific paper
Jan 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21536006f&link_type=abstract
American Astronomical Society, AAS Meeting #215, #360.06; Bulletin of the American Astronomical Society, Vol. 42, p.548
Statistics
Computation
Scientific paper
X-ray binaries are unique astrophysical laboratories as they carry information about many complex physical processes such as star formation, compact object formation, and evolution of interacting binary systems. Motivated by deep Chandra observations of extra-galactic populations of X-ray binaries, I will present population studies of low-mass X-ray binaries in elliptical galaxies. These simulations are targeted at understanding the origin of the shape and normalization of the observed X-ray luminosity functions as well as the transient behavior of X-ray binaries. Finally, I will briefly talk about an ongoing project towards developing a new advanced computational tool for the study of X-ray binary populations formed in both galactic fields and dense stellar clusters.
Fabbiano Giuseppina
Fragos Tassos
Kalogera Vassiliki
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