Speaker
Anastasia Kilina
(IRAP)
Description
Ultraluminous X-ray sources (ULXs) are accreting stellar compact objects whose X-ray luminosities exceed the Eddington limit. In order to get more insights on the nature of their accreting compact object (black hole or neutron star) and the geometries of super-Eddington accretion flows, it is useful to look at the influence of ULXs on their environment. I will present how VLT/MUSE 3-D spectroscopy can help studying bubbles of ionized gas formed around some ULXs. I will discuss the nature of those bubbles: ionization by X-ray radiation and/or shocks which would indicate the presence of winds.
Contribution | Oral talk |
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Affiliation | IRAP |
akilina@irap.omp.eu |
Author
Anastasia Kilina
(IRAP)
Co-author
Olivier Godet
(IRAP)