Hostname: page-component-78c5997874-lj6df Total loading time: 0 Render date: 2024-11-18T09:17:08.608Z Has data issue: false hasContentIssue false

Some Features in the Spectra of Extragalactic Radio Sources

Published online by Cambridge University Press:  25 April 2016

O. B. Slee*
Affiliation:
Division of Radiophysics, CSIRO, Sydney

Extract

A recent analysis of the spectra of about 2000 sources in the Culgoora-3 list (Slee 1977) of radio sources (Slee et al. 1981) has revealed some interesting features which may be the result of source evolution. The Culgoora-3 spectra were obtained by combining the 80 and 160 MHz flux densities from the Culgoora radioheliograph with other published flux data between 10 and 10,000 MHz; this is probably the most accurate set of spectra yet derived for a large number of sources selected for observation in a reasonably consistent manner. In addition to fitting the log S-log v data for each source with a straight line (its slope is the usual definition of spectral index) Slee et al. also fitted second-degree and third-degree polynomials to search for curvature in the spectra.

Type
Contributions
Copyright
Copyright © Astronomical Society of Australia 1981

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Gower, J. F. R. Mon. Not. R. Astron. Soc., 133, 151 (1966).Google Scholar
Katgert-Merkelijn, J., Lari, C., and Padrielli, L. Astron. Astrophys. Suppl. Ser., 40, 91 (1980).Google Scholar
Slee, O. B. Aust. J. Phys. Astrophys. Suppl. No. 43 (1977).Google Scholar
Slee, O. B., Siegman, B., and Mulhall, P. (in preparation) (1981).Google Scholar
Tielens, A. G. G., Miley, G. K., and Willis, A. G. Astron. Astrophys. Suppl., 35, 153 (1979).Google Scholar