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

M. I. Large; A. E. Vaughan

doi:10.1038/220043a0

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 journal › Letter › peer-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 language	English
Pages (from-to)	43-44
Number of pages	2
Journal	Nature
Volume	220
Issue number	5162
DOIs	https://doi.org/10.1038/220043a0
Publication status	Published - 1968
Externally published	Yes

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@article{42d0877b01c34ccaa8743c441cfa4d90,

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

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.",

author = "Large, {M. I.} and Vaughan, {A. E.}",

year = "1968",

doi = "10.1038/220043a0",

language = "English",

volume = "220",

pages = "43--44",

journal = "Nature",

issn = "0028-0836",

publisher = "Nature Publishing Groups",

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T1 - Dispersion and pulse length of the pulsating radio source PSR 1749-28 [1]

AU - Large, M. I.

AU - Vaughan, A. E.

PY - 1968

Y1 - 1968

N2 - 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.

AB - 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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U2 - 10.1038/220043a0

DO - 10.1038/220043a0

M3 - Letter

AN - SCOPUS:36949044412

SN - 0028-0836

VL - 220

SP - 43

EP - 44

JO - Nature

JF - Nature

IS - 5162

ER -

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

Abstract

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