The Radio Pulsar J0205+6449 in the SNR 3C 58

Pulsed radio emission has been detected from the X-ray pulsar J0205+6449 in the SNR 3C 58 at 111 and 88 MHz on radio telescopes of the Pushchino Radio Astronomy Observatory. The dispersion measure DM = 141 pc cm−3 has been confirmed. The synchrotron mechanism is proposed for the radio and X-ray emission to explain the lower X-ray and radio luminosities of this pulsar compared to the Crab pulsar.

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The large synthesis radio telescopes of the National Radio Astronomy Observatory

1992 IEEE Microwave Symposium Digest MTT-S ◽

10.1109/mwsym.1992.188225 ◽

2003 ◽

Cited By ~ 2

Author(s):

P.J. Napier

Keyword(s):

Radio Astronomy ◽

Radio Telescopes ◽

Astronomy Observatory ◽

Radio Astronomy Observatory

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Radio Emission Of The Nuclei Of Barred Spiral Galaxies

Australian Journal of Physics ◽

10.1071/ph660883 ◽

1966 ◽

Vol 19 (6) ◽

pp. 883 ◽

Cited By ~ 7

Keyword(s):

Radio Emission ◽

Radio Telescope ◽

Radio Astronomy ◽

Spiral Galaxies ◽

Astronomy Observatory ◽

Radio Observations ◽

Barred Galaxies ◽

Radio Astronomy Observatory ◽

Barred Spiral Galaxies

The results of radio observations of 98 barred galaxies at 11, 21, and 75 cm are presented. The observations were carried out with the 210 ft radio telescope of the Australian National Radio Astronomy Observatory and with the Mills Cross of the Sydney Uni

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Variable Radio Emission from X-Ray Sources

International Astronomical Union Colloquium ◽

10.1017/s0252921100032905 ◽

1971 ◽

Vol 15 ◽

pp. 173-175 ◽

Cited By ~ 1

Author(s):

L. L. E. Braes ◽

G. K. Miley

Keyword(s):

Radio Emission ◽

Aperture Synthesis ◽

Electromagnetic Spectrum ◽

Radio Telescopes ◽

Low Resolution ◽

X Ray ◽

Synthesis Technique ◽

Variable Radio

Dr. KELLOGG has just described some exciting new observations of X-ray sources made with the UHURU satellite. We shall now move some nine orders of magnitude in wavelength to the opposite end of the electromagnetic spectrum and report measurements of weak radio emission from some of the objects he mentioned. For the detection of weak sources most radio telescopes are not noise limited, but are confusion limited by their low resolution. The aperture synthesis technique minimizes this problem because it enables one to pinpoint the position of weak sources to the order of one second of arc.

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Design, environmental and sustainability constraints of new African observatories: The example of the Mozambique Radio Astronomy Observatory

2013 Africon ◽

10.1109/afrcon.2013.6757829 ◽

2013 ◽

Author(s):

Domingos Barbosa ◽

Miguel Bergano ◽

Valerio A. R. M. Ribeiro ◽

Anita Loots ◽

Venkatasubramani L. Thondikulam ◽

...

Keyword(s):

Radio Astronomy ◽

Astronomy Observatory ◽

Radio Astronomy Observatory

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On the peculiarities in the spin-down of isolated radio pulsars

Proceedings of the International Astronomical Union ◽

10.1017/s1743921312023666 ◽

2012 ◽

Vol 8 (S291) ◽

pp. 208-208

Author(s):

Augustine Chukwude

Keyword(s):

Radio Astronomy ◽

Time Resolution ◽

Local Phase ◽

Astronomy Observatory ◽

Radio Pulsars ◽

Short Term ◽

Radio Astronomy Observatory ◽

Long Term Changes ◽

Timing Data

AbstractWe investigate the spin-down behaviour of a sample of 25 radio pulsars on decadal timescales (~ 18 years) using a continuous timing data obtained over a period of at Hartebeesthoek Radio Astronomy Observatory (HartRAO). Particular attention is placed on achieving a better time resolution of both the short-term and long-term changes in pulsar spin-down using local phase-coherent measurements of the spin-down rates (). We demonstrate that the spin-down of radio pulsars is generally complicated by a superposition of processes that may or may not be related. Specifically, our results show that (i) for 7 pulsars, the observed spin-down variation is largely stochastic, characterized by random and sustained jumps in of varying amplitudes, (ii) for 9 objects, the spin-down evolution shows dominant monotonic variations in superimposed on short-term stochastic jumps in the parameter, and (iii) for the remaining 9 pulsars, the long-term spin-down evolution is non-monotonic, dominated by some systematic excursion in the measured spin-down rates.

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