Hostname: page-component-cd9895bd7-p9bg8 Total loading time: 0 Render date: 2024-12-26T02:19:40.675Z Has data issue: false hasContentIssue false
  • English
  • Français

31. Apparent intensity variations of the radio source Hydra A

Published online by Cambridge University Press:  14 August 2015

J. G. Bolton  and
O. B. Slee
J. G. Bolton
Affiliation:
Radiophysics Laboratory, Commonwealth Scientific and Industrial Research Organisation, Sydney, Australia
O. B. Slee
Affiliation:
Radiophysics Laboratory, Commonwealth Scientific and Industrial Research Organisation, Sydney, Australia

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

During the course of a survey for radio sources using a sea interferometer changes in the apparent intensity of the source Hydra A were observed. The intensities on two consecutive days differed by more than 30 % although the intensities of sources appearing earlier and later on the same records showed no significant changes. The position of this source given by Mills (1952) [2] is r.a. 09h 15m 46s, dec. − 11° 55′ (epoch 1950) and its I.A.U. number 09S1A.

Type
Part II: Point Sources: Individual Study and Physical Theory
Information
Symposium - International Astronomical Union , Volume 4: Radio Astronomy , 1957 , pp. 174 - 178
Copyright
Copyright © Cambridge University Press 1957 

References

1. Slee, O. B. Aust. J. Phys. 8, 487, 1955.Google Scholar
2. Mills, B. Y. Aust. J. Sci. Res. A , 5, 266, 1952.Google Scholar
3. Mills, B. Y., Little, A. G. and Sheridan, K. V. (in preparation). ‘A high resolution radio telescope for use at a wave-length of 3·5 metres.’ Google Scholar