Results 11 to 20 of about 5,289 (173)
Radio Emission from an Ultraluminous X-Ray Source [PDF]
The physical nature of ultraluminous x-ray sources is uncertain. Stellar mass black holes with beamed radiation and intermediate mass black holes with isotropic radiation are two plausible explanations.
Corbel, Stephane +3 more
core +6 more sources
Long-term X-ray Variability of Ultraluminous X-ray Sources [PDF]
Long-term X-ray modulations on timescales from tens to hundreds of days have been widely studied for X-ray binaries located in the Milky Way and the Magellanic Clouds.
Chou, Y. +5 more
core +6 more sources
Observations of ultraluminous X-ray sources [PDF]
Ultraluminous X-ray sources (ULXs), first observed ~30 years ago, have been argued as extreme stellar mass black hole binaries or a new class intermediate mass black hole.
Gladstone, Jeanette Claire
core +2 more sources
Ultraluminous X-ray Sources and Their Nebulae [PDF]
One of the interesting features of Ultraluminous X-ray sources is that many of them are surrounded by luminous nebulae exhibiting diverse observational properties. In different cases the nebulae are photoionized or shock-powered.
Magnus Axelsson, Pavel Abolmasov
core +3 more sources
Nature of the Extreme Ultraluminous X-ray Sources [PDF]
In this proof-of-concept study we demonstrate that in a binary system mass can be transferred toward an accreting compact object at extremely high rate. If the transferred mass is efficiently converted to X-ray luminosity (with disregard of the classical
Belczynski, Krzysztof +3 more
core +5 more sources
Compact radio emission in Ultraluminous X-ray sources [PDF]
We present results from our studies of radio emission from selected Ultraluminous X-ray (ULX) sources, using archival Giant Metrewave Radio Telescope (GMRT) data and new European VLBI Network (EVN) observations.
Becker +14 more
core +2 more sources
Ultraluminous X-ray Sources and Star Formation [PDF]
Chandra observations of the Cartwheel galaxy reveal a population of ultraluminous X-ray sources (ULXs) with lifetimes < 10^7 yr associated with a spreading wave of star formation which began some 3 x 10^8 yr ago.
King, Andrew R.
core +3 more sources
X-ray reflection in a sample of X-ray bright Ultraluminous X-ray sources [PDF]
We apply a reflection-based model to the best available XMM-Newton spectra of X-ray bright UltraLuminous X-ray (ULX) sources (NGC 1313 X-1, NGC 1313 X-2, M 81 X-6, Holmberg IX X-1, NGC 5408 X-1 and Holmberg II X-1).
A. C. Fabian +52 more
core +2 more sources
Spectral variability of ultraluminous X-ray sources [PDF]
We study spectral variability of 11 ultraluminous X-ray sources (ULX) using archived XMM-Newton and Chandra observations. We use three models to describe the observed spectra; a power-law, a multi-colour disk (MCD) and a combination of these two models ...
Abolmasov +60 more
core +4 more sources
Ultraluminous X-Ray Sources [PDF]
32 pages, 21 figures, 1 ...
Fabrika S.N. +3 more
openaire +2 more sources

