- Abstract:
-
Recent investigations of how the median size of extragalactic radio sources change with redshift have produced inconsistent results. Eales compared the radio and optical properties of a bright 3C and faint 6C sample and concluded that $D\propto(1+z)^{-1.1\pm0.5}$ ($\Omega_0 = 0$), with $D$ being the median size of the radio sources at a given epoch and z the redshift. Oort, Katgert, and Windhorst, on the other hand, from a comparison of the properties of a number of radio samples, found much ...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1086/176201
-
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- Journal:
- ASTROPHYSICAL JOURNAL
- Volume:
- 451
- Issue:
- 1
- Pages:
- 76-87
- Publication date:
- 1995-08-08
- DOI:
- EISSN:
-
1538-4357
- ISSN:
-
0004-637X
- URN:
-
uuid:aa8c2e60-b0fc-45ab-9d23-9f9b882c08cc
- Source identifiers:
-
17135
- Local pid:
- pubs:17135
- Keywords:
- Copyright date:
- 1995
- Notes:
-
compressed and uuencoded postscript file. 33 pages including 5
figures (441951 bytes). Accepted for publication in September ApJ
Journal article
The Linear-Size Evolution of Classical Double Radio Sources
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