SPECTROSCOPIC SIGNATURES OF THE SUPERORBITAL PERIOD IN THE NEUTRON STAR BINARY LMC X-4

We present the first high-resolution X-ray study of emission line variability with superorbital phase in the neutron star binary LMC X-4. Our analysis provides new evidence from X-ray spectroscopy confirming accretion disk precession as the origin of the superorbital period. The spectra, obtained wi...

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Bibliographic Details
Main Authors: Neilsen, Joseph M. G. (Author), Lee, Julia C. (Author), Nowak, Michael A. (Contributor), Dennerl, Konrad (Author), Vrtilek, Saeqa Dil (Author)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: Institute of Physics/American Astronomical Society, 2015-03-30T17:21:01Z.
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