Online Resource
Cambridge University Press (CUP)
;
1996
In:
Symposium - International Astronomical Union Vol. 175 ( 1996), p. 585-587
In:
Symposium - International Astronomical Union, Cambridge University Press (CUP), Vol. 175 ( 1996), p. 585-587
Abstract:
The Hubble diagram of GPS galaxies has a low dispersion and a steep slope compared with that for 3C galaxies. The relative faintness of GPS galaxies at high redshift may be due to the absence of the aligned optical/uv component seen in high redshift 3C galaxies. The GPS Hubble relation is too steep to fit with evolution models for passively evolving ellipticals. This could be caused by the dynamical evolution of the GPS galaxies.
Type of Medium:
Online Resource
ISSN:
0074-1809
DOI:
10.1017/S0074180900081936
Language:
English
Publisher:
Cambridge University Press (CUP)
Publication Date:
1996
SSG:
16,12
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