THE CLOSE STELLAR COMPANIONS TO INTERMEDIATE-MASS BLACK HOLES
ASTROPHYSICAL JOURNAL
Authors: MacLeod, Morgan; Trenti, Michele; Ramirez-Ruiz, Enrico
Abstract
When embedded in dense cluster cores, intermediate-mass black holes (IMBHs) acquire close stellar or stellarremnant companions. These companions are not only gravitationally bound, but also tend to hierarchically isolate from other cluster stars through series of multibody encounters. In this paper we study the demographics of IMBH companions in compact star clusters through direct N-body simulations. We study clusters initially composed of 10(5) or 2 x 10(5) stars with IMBHs of 75 and 150 solar masses, and we follow their evolution for 6-10 Gyr. A tight, innermost binary pair of IMBH and stellar object rapidly forms. The IMBH has a companion with an orbital semimajor axis at least three times tighter than the second-most-bound object over 90% of the time. These companionships have typical periods on the order of years and are subject to cycles of exchange and destruction. The most frequently observed, long-lived pairings persist for similar to 10(7) years. The demographics of IMBH companions in clusters are diverse: they include both main-sequence, giant stars and stellar remnants. Companion objects may reveal the presence of an IMBH in a cluster in one of several ways. The most-bound companion stars routinely suffer grazing tidal interactions with the IMBH, offering a dynamical mechanism to produce repeated flaring episodes like those seen in the IMBH candidate HLX-1. The stellar winds of companion stars provide a minimum quiescent accretion rate for IMBHs, with implications for radio searches for IMBH accretion in globular clusters. Finally, gravitational wave inspirals of compact objects occur with promising frequency.
Regulatory gene expression patterns reveal transverse and longitudinal subdivisions of the embryonic zebrafish forebrain
MECHANISMS OF DEVELOPMENT
Authors: Hauptmann, G; Gerster, T
Abstract
To shed light on the organization of the rostral embryonic brain of a lower vertebrate, we have directly compared the expression patterns of dlx, fgf, hh, hlx, otx, pas, POU, winged helix and wnt gene family members in the fore- and midbrain of the zebrafish. We show that the analyzed genes are expressed in distinct transverse and longitudinal domains and share expression boundaries at stereotypic positions within thr fore- and midbrain. Some of these shared expression boundaries coincide with morphological landmarks like the pathways of primary axon tracts. We identified a series of right transverse diencephalic domains suggestive of neuromeric subdivisions within the rostral brain. in addition, we identified four molecularly distinct longitudinal subdivisions and provide evidence for a strong bending of the longitudinal rostral brain axis at the cephalic flexure. our data suggest a strong conservation of early forebrain organization between lower and higher vertebrates. (C) 2000 Elsevier Science Ireland Ltd. All rights reserved.