Abstract
THE strongly variable X-ray source Cen XR-2 was first observed from rocket payloads of the Universities of Adelaide and Tasmania (UAT) in April 1967. This letter reports the results of a reanalysis of UAT flight II on April 20, 1967. It is shown that the particular rocket motion coupled with the unique intensity of Cen XR-2 at the time permits determination of a galactic longitude for the source lII = 310.2±1°, which is relatively insensitive to possible errors in the rocket attitude solution. A comparison with more recent X-ray and optical observations yields a positional conflict suggestive of two separate X-ray phenomena.

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FRANCEY, R. Position of Cen XR-2 (April 1967). Nature Physical Science 229, 229–233 (1971). https://doi.org/10.1038/physci229229a0
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DOI: https://doi.org/10.1038/physci229229a0
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