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...
Main Authors: | , , , , , , |
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Other Authors: | |
Format: | Article |
Language: | en_US |
Published: |
IOP Publishing
2015
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Online Access: | http://hdl.handle.net/1721.1/93133 |