2015A&A...579A..33V


C.D.S. - SIMBAD4 rel 1.7 - 2020.07.08CEST02:05:55

2015A&A...579A..33V - Astronomy and Astrophysics, volume 579A, 33-33 (2015/7-1)

Population synthesis of classical low-mass X-ray binaries in the Galactic Bulge.

VAN HAAFTEN L.M., NELEMANS G., VOSS R., VAN DER SLUYS M.V. and TOONEN S.

Abstract (from CDS):

We model the present-day population of classical low-mass X-ray binaries (LMXBs) with neutron star accretors, which have hydrogen-rich donor stars. Their population is compared with that of hydrogen-deficient LMXBs, known as ultracompact X-ray binaries (UCXBs). We model the observable LMXB population and compare it to observations. We model the Galactic Bulge because it contains a well-observed population and it is the target of the Galactic Bulge Survey. We combine the binary population synthesis code SeBa with detailed LMXB evolutionary tracks to model the size and properties of the present-day LMXB population in the Galactic Bulge. Whether sources are persistent or transient, and what their instantaneous X-ray luminosities are, is predicted using the thermal-viscous disk instability model. We find a population of ∼2.1x103 LMXBs with neutron star accretors. Of these about 15-40 are expected to be persistent (depending on model assumptions), with luminosities higher than 1035erg/s. About 7-20 transient sources are expected to be in outburst at any given time. Within a factor of two these numbers are consistent with the observed population of bright LMXBs in the Bulge. This gives credence to our prediction of the existence of a population of ∼1.6x103 LMXBs with low donor masses that have gone through the period minimum, and have present-day mass transfer rates below 10–11M/yr. Even though the observed population of hydrogen-rich LMXBs in the Bulge is larger than the observed population of (hydrogen-deficient) UCXBs, the latter have a higher formation rate. While UCXBs may dominate the total LMXB population at the present time, the majority would be very faint or may have become detached and produced millisecond radio pulsars. In that case UCXBs would contribute significantly more to the formation of millisecond radio pulsars than hydrogen-rich LMXBs.

Abstract Copyright:

Journal keyword(s): binaries: close - Galaxy: bulge - X-rays: binaries

Simbad objects: 7

goto Full paper

goto View the reference in ADS

Number of rows : 7

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 M 31 G 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 10903 1
2 PSR J1023+0038 LXB 10 23 47.6840307966 +00 38 41.006983532     17.31     GV 308 0
3 M 105 LIN 10 47 49.600 +12 34 53.87   10.56 9.76 9.12 8.18 ~ 1379 0
4 NGC 4278 LIN 12 20 06.82563 +29 16 50.7124 11.54 11.09 10.16     ~ 887 2
5 NAME Gal Center reg 17 45 40.04 -29 00 28.1           ~ 11535 0
6 NAME MW Group GrG ~ ~           ~ 14 0
7 NAME Galactic Bulge reg ~ ~           ~ 3389 0

    Equat.    Gal    SGal    Ecl

To bookmark this query, right click on this link: simbad:objects in 2015A&A...579A..33V and select 'bookmark this link' or equivalent in the popup menu


2020.07.08-02:05:55

© Université de Strasbourg/CNRS

    • Contact