J/A+AS/132/31 J/A+AS/132/31 Kinematical models for double radio sources K Nilsson Astron. Astrophys. Suppl. Ser. 132 31 1998 1998A&AS..132...31N VIII/15 : Parkes Radio Sources Catalogue (PKSCAT90) (Wright+ 1990) VIII/17 : The 1.4GHz Northern Sky Catalog (White+ 1992) VIII/16 : Molonglo Reference Catalogue of Radio Sources (Large+ 1991) VIII/4 : Fourth Cambridge Survey (4C) (Pilkington+ 1965; Gower+1967) VIII/43 : Radio survey of clusters of galaxies (Andernach+ 1978) VIII/13 : A new catalog of 53522 4.85GHz sources (Becker+ 1991) VII/2 : Master list of radio sources, updated 1978 (Dixon, 1970) VIII/5 : Bright Extragalactic Radio Sources (1Jy) (Kuehr+, 1981) VII/99 : Radial Velocities of Galaxies (Palumbo+ 1986) III/175 : Optical spectroscopy of radio sources (Stickel+, 1989-94) J/ApJS/81/83 : Compendium of Radio Spectra and Luminosities (Herbig+ 1992) Baryshev & Teerikorpi, Paper I. 1995A&A...295...11B Radio sources galaxies: active ISM: jets radio continuum: galaxies These tables contain structural parameters for a large sample of classical FR II (Fanaroff-Riley II, 1974MNRAS.167p..31F) double radio sources obtained from the literature.

IAU IAU name of the source --- m_IAU Multiplicity index on IAU --- Name Other name of the source --- z Redshift of optical identification --- LAS Largest angular size of the radio structure arcsec SI Spectral index between 178MHz and 5GHz --- Sizel Projected linear size number=1 H_0_=50km/s/Mpc and q_0_=0.5 is assumed kpc logL Luminosity between 10MHz and 10GHz in the rest frame of the source number=1 H_0_=50km/s/Mpc and q_0_=0.5 is assumed [10-7W] S5GHZcore Flux of the core at 5 GHz mJy SIcore Spectral index of the core near 5 GHz --- Pc/Ptot Relative strength of the core at 5 GHz number=1 H_0_=50km/s/Mpc and q_0_=0.5 is assumed --- Q Arm length ratio number=2 Ratio fo the distances of the outermost hotspots at opposite sides from the radio core or the optical identification. Q>1 by definition --- D Bending angle deg F Lobe flux ratio number=3 F=S1/S2, where S1 is the flux density of the lobe farther from the core and S2 is the flux density of the lobe loser to the core --- nuF Frequency at which F has been measured MHz Flux% Interferometric flux/single dish flux number=4 Flux%=(Score+Slobes)/Stot, where Score is the flux density of the core, Slobes=S1+S2 is the flux density of the lobes and Stot is the total flux density of the source measured with a single dish radio telescope --- ID Optical identification number=5 'G': galaxy 'Q': Quasar ' ': unidentified --- Refmap Reference of the radio map (in refs.dat) --- n_Refmap Note on Refmap number=6 *: No actual radio map was available and the structural data was taken from tabular material --- Refs References in refs.dat file --- Sample Sample membership --- Ref Reference number --- BibCode BibCode --- Aut Authors name --- Com Comments --- Patricia Bauer CDS 1998May15Kari Nilsson <kani@deneb.astro.utu.fi> J_A+AS_132_31.xml