The X-ray light curve of 4U 2129+47
1980
We present the light curve of 4U 2129+47 and show that it almost certainly has a period of approx.0.22 days. This is the same period as the optical candidate proposed by Thorstensen et al. Binary X-ray source models, consisting of an M dwarf plus either a neutron star or a white dwarf, are briefly discussed.
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