Compact X-ray binaries in and out of core collapsed globulars

We review new Chandra and HST observations of the core collapsed cluster NGC 6397 as a guide to understanding the compact binary (CB) populations in core collapse globulars. New cataclysmic variables (M) and main sequence chromospherically active binaries (ABs) have been identified, enabling a larger sample for comparison of the L-x, F-x/F-V, and X-ray vs. optical color distributions. Comparison of the numbers of CBs with L-x greater than or similar to 10(31) erg s(-1) in 4 core collapse vs. 12 King model clusters reveals that the specific frequency S-X (number of CBs per unit cluster mass) is enhanced in core collapse Clusters, even when normalized for their stellar encounter rate. Although core collapse is halted by the dynamical heating due to stellar (and binary) interaction with CBs in the core, we conclude that production of the hardest CBs - especially CVs - is enhanced during core collapse. NGC 6397 has its most luminous CVs nearest the cluster center, with two newly discovered very low luminosity (old, quiescent) CVs far from the core. The active binaries as well as neutron star systems (MSP and qLMXB) surround the central core. The overall CB population appears to be asymmetric about the cluster center, as in several other core collapse clusters observed with Chandra, suggesting still poorly understood scattering processes. (C) 2006 COSPAR. Published by Elsevier Ltd. All rights reserved.