A NEW DYNAMICAL MODEL FOR THE BLACK HOLE BINARY LMC X-1
We present a dynamical model of the high mass X-ray binary LMC X-1 based on high-resolution optical spectroscopy and extensive optical and near-infrared photometry. From our new optical data we find an orbital period of P = 3.90917 ± 0.00005 days. We present a refined analysis of the All Sky Monitor...
Main Authors: | , , , , , , , , , , , , |
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Other Authors: | , , |
Format: | Article |
Language: | English |
Published: |
Institute of Physics/American Astronomical Society,
2015-03-19T19:17:57Z.
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Subjects: | |
Online Access: | Get fulltext |