1997A&A...326..130M


Query : 1997A&A...326..130M

1997A&A...326..130M - Astronomy and Astrophysics, volume 326, 130-138 (1997/10-1)

Clues on the nature of Compact Steep Spectrum radio sources from optical spectroscopy.

MORGANTI R., TADHUNTER C.N., DICKSON R. and SHAW M.

Abstract (from CDS):

New long-slit spectra are presented for a group of Compact-Steep-Spectrum (CSS) sources (i.e. powerful radio sources with sub-galactic size and steep spectral index at high radio frequencies) selected from the southern (δ< 10°) 2-Jy sample of radio sources with redshift limit of z=0.7. Their spectra are strong in emission lines (e.g. [O III]λ5007 and [O II]λ3727), as expected for such powerful radio sources. The line luminosities and ratios obtained for these compact sources are compared with those for the other sources of the southern 2-Jy sample. We find that the optical spectra for the CSS sources show characteristics very similar to the extended sources of similar radio power and redshift. In particular, we find that the CSS sources follow the correlation between the radio power and [O III]λ5007 and [O II]λ3727 luminosities found for the extended sources, although there is tentative evidence that they have lower [O III]λ5007 luminosities. Also, the optical continuum spectral energy distribution (SED) and polarization properties of the CSS sources show the same variety of characteristics observed among the extended sources. The first-order similarity that we find between the spectra of CSS sources and the extended sources of similar radio power is consistent with the idea that the CSS sources are young radio sources in which the radio jets have yet to emerge from the central regions of the host galaxies.

Abstract Copyright:

Journal keyword(s): galaxies: active - galaxies: nuclei - radio continuum: galaxies

Simbad objects: 10

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Number of rows : 10
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 QSO B0023-263 BLL 00 25 49.15629900 -26 02 12.6141092   20.30 19.5 18.084   ~ 161 1
2 4C 31.04 rG 01 19 35.00087601 +32 10 50.0619670   16 14.5     ~ 235 1
3 ICRF J025246.1-710435 AGN 02 52 46.15578 -71 04 35.2742   19.0 19.0     ~ 96 1
4 ICRF J115421.7-350529 Sy1 11 54 21.7842834888 -35 05 29.079469716   18.81 17.84     ~ 129 1
5 NGC 4690 GiG 12 47 55.5227576592 -01 39 21.805729344   14.0       ~ 61 0
6 PKS 1306-09 rG 13 08 39.1573432224 -09 50 32.424542340   20.767 20.500 18.439   ~ 76 1
7 UGC 9799 Sy2 15 16 44.4893939136 +07 01 17.825410740   15.19 14.17     ~ 446 3
8 ICRF J181935.0-634548 Sy2 18 19 35.00241 -63 45 48.1926   16.80 14.40 13.4   ~ 146 1
9 ICRF J193925.0-634245 Sy2 19 39 25.0245304992 -63 42 45.640373400   18.87 18.37 17.64   ~ 1225 1
10 ICRF J213750.0-204231 Sy1 21 37 50.00785656 -20 42 31.6728477   20.400 19.4 19.286   ~ 95 1

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