MODELING THE OPTICAL-X-RAY ACCRETION LAG IN LMC X-3: INSIGHTS INTO BLACK-HOLE ACCRETION PHYSICS

The X-ray persistence and characteristically soft spectrum of the black hole X-ray binary LMC X-3 make this source a touchstone for penetrating studies of accretion physics. We analyze a rich, ten-year collection of optical/infrared (OIR) time-series data in conjunction with all available contempora...

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Bibliographic Details
Main Authors: Steiner, James F., McClintock, Jeffrey E., Orosz, Jerome A., Buxton, Michelle, Bailyn, Charles D., Kara, Erin, Remillard, Ronald A
Other Authors: MIT Kavli Institute for Astrophysics and Space Research
Format: Article
Language:en_US
Published: IOP Publishing 2015
Online Access:http://hdl.handle.net/1721.1/93133