Volume 525, January 2011
|Number of page(s)||5|
|Section||Catalogs and data|
|Published online||29 November 2010|
An optical spectroscopic survey of the 3CR sample of radio galaxies with z < 0.3
III. Completing the sample⋆
INAF, Osservatorio Astronomico di Padova,
2 SISSA-ISAS, via Beirut 2-4, 34014 Trieste, Italy
3 INAF - Osservatorio Astronomico di Torino, Strada Osservatorio 20, 10025 Pino Torinese, Italy
4 School of Mathematical and Physical Sciences, University of Sussex, Falmer, Brighton BN1 9RH, UK
5 Department of Physics, Rochester Institute of Technology, 85 Lomb Memorial Drive, Rochester, NY 14623, USA
6 Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
7 INAF - Istituto di Radio Astronomia, via P. Gobetti 101, 40129 Bologna, Italy
Received: 12 August 2010
Accepted: 4 October 2010
We present optical nuclear spectra for nine 3CR radio sources obtained with the Telescopio Nazionale Galileo, that complete our spectroscopic observations of the sample up to redshifts <0.3. We measure emission line luminosities and ratios, and derive a spectroscopic classification for these sources.
Key words: galaxies: active / galaxies: jets / galaxies: elliptical and lenticular, cD / galaxies: nuclei
© ESO, 2010
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