| Issue |
A&A
Volume 525, January 2011
|
|
|---|---|---|
| Article Number | A28 | |
| Number of page(s) | 5 | |
| Section | Catalogs and data | |
| DOI | https://doi.org/10.1051/0004-6361/201015574 | |
| Published online | 29 November 2010 | |
An optical spectroscopic survey of the 3CR sample of radio galaxies with z < 0.3
III. Completing the sample⋆
1
INAF, Osservatorio Astronomico di Padova,
Vicolo dell’Osservatorio
5,
35122
Padova,
Italy
e-mail: sara.buttiglione@oapd.inaf.it
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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