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The Linear-Size Evolution of Classical Double Radio Sources

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 ...

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Publication status:
Published

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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:

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