Low-Mass X-ray Binary Models for NGC3379 and NGC4278

Details Low-Mass X-ray Binary Models for NGC3379 and NGC4278 Low-Mass X-ray Binary Models for NGC3379 and NGC4278

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...20915501f&link_type=abstract

2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #155.01; Bulletin of the American Astronomical Society,

Astronomy and Astrophysics

Astronomy

Scientific paper

We present theoretical models for populations of Low-Mass X-Ray Binaries in two elliptical galaxies NGC3379 and NGC4278. The models are calculated with the recently updated StarTrack code (Belczynski et al. 2006) and targeted to modeling and understanding the origin of the shape characteristics of the X-ray luminosity functions (XLF) in these galaxies. For the first time we explore the population XLF down to low luminosities in the range of (5-10)E36 erg/s as probed by the most recent observational results (Kim et al. 2006).

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