SIMBAD references

2009ApJ...707..870B - Astrophys. J., 707, 870-877 (2009/December-3)

On the apparent lack of Be X-ray binaries with black holes.

BELCZYNSKI K. and ZIOLKOWSKI J.

Abstract (from CDS):

In our Galaxy there are 64 Be X-ray binaries known to date. Out of these, 42 host a neutron star (NS), and for the remainder the nature of the companion is unknown. None, so far, are known to host a black hole (BH). There seems to be no apparent mechanism that would prevent formation or detection of Be stars with BHs. This disparity is referred to as a missing Be-BH X-ray binary problem. We point out that current evolutionary scenarios that lead to the formation of Be X-ray binaries predict that the ratio of binaries with NSs to the ones with BHs is rather high, FNStoBH∼ 10-50, with the more likely formation models providing the values at the high end. The ratio is a natural outcome of (1) the stellar initial mass function that produces more NSs than BHs and (2) common envelope evolution (i.e., a major mechanism involved in the formation of interacting binaries) that naturally selects progenitors of Be X-ray binaries with NSs (binaries with comparable mass components have more likely survival probabilities) over ones with BHs (which are much more likely to be common envelope mergers). A comparison of this ratio (i.e., FNStoBH∼ 30) with the number of confirmed Be-NS X-ray binaries (42) indicates that the expected number of Be-BH X-ray binaries is of the order of only ∼0-2. This is entirely consistent with the observed Galactic sample.

Abstract Copyright:

Journal keyword(s): binaries: close - black hole physics - stars: evolution - stars: neutron

Simbad objects: 70

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2009ApJ...707..870B and select 'bookmark this link' or equivalent in the popup menu


2021.04.21-10:46:51

© Université de Strasbourg/CNRS

    • Contact