Cygnus A and Other 3CR Sources in Cosmological Tests
Powerful extended radio galaxies like Cygnus A can be used for cosmological tests. The characteristic, time-independent length \(D_*\) for several radio sources is calculated and compared to the average physical length for a sample of radio galaxies. The ratio of these two lengths as a function of r...
Saved in:
Published in | arXiv.org |
---|---|
Main Authors | , |
Format | Paper |
Language | English |
Published |
Ithaca
Cornell University Library, arXiv.org
12.06.1995
|
Subjects | |
Online Access | Get full text |
Cover
Loading…
Summary: | Powerful extended radio galaxies like Cygnus A can be used for cosmological tests. The characteristic, time-independent length \(D_*\) for several radio sources is calculated and compared to the average physical length for a sample of radio galaxies. The ratio of these two lengths as a function of redshift is used to constrain cosmological parameters. Cygnus A is the only low-redshift (\(z<0.5\)) radio galaxy for which we have an estimate for \(D_*\). We comment on the sensitivity to this one low-redshift point, and results including and excluding Cygnus A are shown. A low density universe is favored, and the one free model parameter is relatively well constrained. |
---|---|
ISSN: | 2331-8422 |