SIMBAD references

2008MNRAS.386..543P - Mon. Not. R. Astron. Soc., 386, 543-552 (2008/May-1)

Optical emission from massive donors in ultraluminous X-ray source binary systems.

PATRUNO A. and ZAMPIERI L.

Abstract (from CDS):

We present evolutionary tracks of binary systems with high-mass companion stars and stellar-through-intermediate mass black holes (BHs). Using Eggleton's stellar evolution code, we compute the luminosity produced by accretion from the donor during its entire evolution. We compute also the evolution of the optical luminosity and colours of the binary system taking the disc contribution and irradiation effects into account. The calculations presented here can be used to constrain the properties of the donor stars in ultraluminous X-ray sources by comparing their position on the Hertzsprung-Russell or colour-magnitude diagrams with the evolutionary tracks of massive BH binaries. This approach may actually provide interesting clues also on the properties of the binary system itself, including the BH mass. We found that, on the basis of their position on the colour-magnitude diagram, some of the candidate counterparts considered can be ruled out and more stringent constraints can be applied to the donor masses.

Abstract Copyright: ©2008 The Authors. Journal compilation © 2008 RAS

Journal keyword(s): galaxies: individual: M81 - galaxies: individual: NGC1313 - galaxies: individual: NGC4559 - galaxies: individual: Holmberg II - X-rays: binaries - X-rays: galaxies

Simbad objects: 12

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2008MNRAS.386..543P and select 'bookmark this link' or equivalent in the popup menu


2019.10.14-07:06:51

© Université de Strasbourg/CNRS

    • Contact