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This article is cited in 1 scientific paper (total in 1 paper)
CONFERENCES AND SYMPOSIA
On the nature of ultraluminous X-ray sources
S. N. Fabrikaab, K. E. Atapinc, A. S. Vinokurova a Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnii Arkhyz, Zelenchukskiy region, Karachai-Cherkessian Republic
b Kazan Federal University
c Lomonosov Moscow State University, Sternberg Astronomical Institute
Abstract:
Ultraluminous X-ray sources (ULXs) that are located in external galaxies exhibit X-ray luminosities exceeding those of the brightest black holes in the Milky Way and the Local Group galaxies by hundreds or even thousands of times. New classes of objects have been discovered: ultraluminous X-ray pulsars (ULXPs) and high-velocity outflows whose X-ray-range speed is up to $0.2c$. The ULXs and ULXPs fully correspond to concepts of super-Eddington accretion. Five ULXs exhibit quasiperiodic oscillations and a flat-topped noise in the X-ray range power spectrum. Optical spectra of ULXs are very similar to those of SS433, late nitrogen stars (WNL/WR), or LBV (luminous blue variable) stars. The results obtained suggest that ULXs are systems that contain supercritical accretion disks.
Received: June 18, 2019 Accepted: April 3, 2019
Citation:
S. N. Fabrika, K. E. Atapin, A. S. Vinokurov, “On the nature of ultraluminous X-ray sources”, UFN, 189:11 (2019), 1240–1248; Phys. Usp., 62:11 (2019), 1162–1169
Linking options:
https://www.mathnet.ru/eng/ufn6520 https://www.mathnet.ru/eng/ufn/v189/i11/p1240
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Abstract page: | 157 | Full-text PDF : | 14 | References: | 14 | First page: | 5 |
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