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Grzegorz Wiktorowicz
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Message 3497 - Posted: 10 May 2019, 4:05:38 UTC

After a series of papers on gravitational wave sources, we published results concerning ultra-luminous X-ray sources. In the paper we analyse the anisotropic emission of radiation from these sources and show that the actual population of ultra-luminous X-ray sources differs from the observed one. Particularly, in flux limited surveys, the observed population will be highly biased toward black hole accretors, whereas neutron star accretors dominate volume-limited observations.

The work can be found here
Grzegorz Wiktorowicz
National Astronomical Observatories,
Chinese Academy of Sciences
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Message boards : News : Emission from ULXs

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