Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-25T14:29:09.990Z Has data issue: false hasContentIssue false
  • English
  • Français

VLBI Observations of 3C298

Published online by Cambridge University Press:  04 August 2017

D. A. Graham  and
L. I. Matveyenko
D. A. Graham
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, F.R.G.
L. I. Matveyenko
Affiliation:
Space Research Institute, Moscow, USSR

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.

The quasar 3C298 (1416+06) has a complex radio-frequency spectrum, with a spectral bend below 100 MHz and a steep slope of −1.2 in the range 150 MHz – 3 GHz. At higher frequencies the spectrum flattens with some evidence of variability.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 110: VLBI and Compact Radio Sources , 1984 , pp. 43 - 44
Copyright
Copyright © Reidel 1984 

References

Anderson, B., Donaldson, W.: 1967, Monthly Notices Roy. Astron. Soc. 137, 81 Google Scholar
Phillips, R.B., Mutel, R.L.: 1982, Astron. Astrophys. 106, 21 Google Scholar