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Skip to Search Results- 12Accretion
- 10Accretion Discs
- 8X-Rays: Binaries
- 4Radio Continuum: Stars
- 4Stars: Neutron
- 3Black Hole Physics
- 11Sivakoff, Gregory Robert
- 6Heinke, Craig O.
- 4Knigge, C.
- 4Miller-Jones, James. C. A.
- 3Altamirano, Diego
- 3Bahramian, Arash
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2017-01-01
Bahramian, Arash, Heinke, Craig O., Tudor, Vlad, Miller-Jones, James. C. A., Bogdanov, Slavko, Maccarone, Thomas J., Knigge, C., Sivakoff, Gregory Robert, Chomiuk, Laura, Strader, Jay, Garcia, Javier A., Kallman, Timothy
47 Tuc X9 is a low-mass X-ray binary (LMXB) in the globular cluster 47 Tucanae, and was previously thought to be a cataclysmic variable. However, Miller-Jones et al. recently identified a radio counterpart to X9 (inferring a radio/X-ray luminosity ratio consistent with black hole LMXBs), and...
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Understanding X-ray irradiation in low-mass X-ray binaries directly from their light-curves
Download2018-01-01
Sivakoff, Gregory Robert, Tetarenko, Bailey E., Dubus, G., Lasota, Jean-Pierre, Heinke, Craig O.
The X-ray light curves of the recurring outbursts observed in low-mass X-ray binaries provide strong test beds for constraining (still) poorly understood disc-accretion processes. These light curves act as a powerful diagnostic to probe the physics behind the mechanisms driving mass inflow and...