Abstract
Turtle and Vaughan1 discovered the pulsar PSR 1749–28 and measured its position coordinates at the Molonglo Radio Observatory. This pulsar is particularly interesting because it is situated only 2 degrees from the direction of the galactic centre. Observations have now been made to determine the frequency drift rate and pulse length of PSR 1749–28.
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References
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LARGE, M., VAUGHAN, A. Dispersion and Pulse Length of the Pulsating Radio Source PSR 1749–28. Nature 220, 43–44 (1968). https://doi.org/10.1038/220043a0
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DOI: https://doi.org/10.1038/220043a0
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