Dispersion and pulse length of the pulsating radio source PSR 1749-28 [1]

M. I. Large*, A. E. Vaughan

*Corresponding author for this work

Research output: Contribution to journalLetterpeer-review

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.

Original languageEnglish
Pages (from-to)43-44
Number of pages2
JournalNature
Volume220
Issue number5162
DOIs
Publication statusPublished - 1968
Externally publishedYes

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