Abstract
It has been suggested that a recently detected galactic center binary X-ray source represents the quiescent state of A1742-289, a transient source which appeared in 1975. We find no evidence for eclipses in the Ariel V RMC data for the transient, suggesting that the binary source is a previously undetected distinct system.
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APA
Kennea, J. A., & Skinner, G. K. (1996). No eclipses in A1742-289 Archival data. Publications of the Astronomical Society of Japan, 48(6). https://doi.org/10.1093/pasj/48.6.L117
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