J/A+AS/106/1 Radio data in Dumbbell galaxies (Gregorini+, 1994) ================================================================================ Dumbbell galaxies and multiple nuclei in rich clusters: radio data Gregorini L., de Ruiter H.R., Parma P., Sadler E.M., Vettolani G., Ekers R.D. =1994A&AS..106....1G ================================================================================ ADC_Keywords: Clusters, galaxy ; Galaxies, radio Keywords: galaxies: clusters - galaxies: elliptical and lenticular, cD - radio continuum: galaxies Post-publication Notes: *14-Oct-1994: following a remark by H. Andernach (heinz@adel.univ-lyon1.fr) on the high value (363.5mJy) of the peak flux of A3432, L. Gregorini (GREGORINI@astbo1.bo.cnr.it) answered: "I had no time to directly check on the map (I am teaching), but from my printed paper I agree with you: the correct value must be a factor of 10 less. Thank you for finding this mistake." File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table4 74 271 Radio sources in the clusters fields table5 81 172 Radio sources identified with the cluster brightest member -------------------------------------------------------------------------------- Byte-per-byte Description of file: table4 table5 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 A6 --- Name Cluster name 8- 9 A2 --- N Reference number of the source; a letter refers to the different components of the extended sources 11- 12 I2 h RAh []? Right ascension 1950.0 (1) 14- 15 I2 min RAm []? Right ascension 1950.0 (1) 17- 21 F5.2 s RAs []? Right ascension 1950.0 (1) 23 A1 --- DE- Declination sign 24- 25 I2 deg DEd []? Declination 1950.0 (1) 27- 28 I2 arcmin DEm []? Declination 1950.0 (1) 30- 33 F4.1 arcsec DEs []? Declination 1950.0 (1) 35 A1 --- l_S6cm limit flag on S6cm 36- 42 F7.2 mJy S6cm []? Total flux density at 6 cm (5 GHz) not corrected for attenuation effects (2) 49- 52 F4.1 arcsec FWHM1 []? Full Width Half Maximun (FWHM) along major axis of a Gaussian fitting of the source 53 A1 --- x [x] An 'x' indicates two values of FWHM along major and minor axes 54 A1 --- l_FWHM2 limit flag for second values of FWHM 55- 59 F5.2 arcsec FWHM2 []? FWHM (along minor axis if x in column 53) 61 A1 --- l_PA limit flag on PA 62- 64 I3 deg PA []? Position angle of a Gaussian fitting the source 66- 68 I3 arcsec LAS []? Largest angular size for complex sources 70- 73 F4.1 arcmin D []? Distance of the source from the pointing position -------------------------------------------------------------------------------- Note (1): in table4, the right ascension and declination refers to the radio emission peak. See also Note (2) below Note (2): in table5, -For non detected radio sources, the right ascension and declination refers to optical position of the dominant galaxy the F value refers to 3 sigma limit for the flux; -For the detected radio sources, the right ascension and declination of the first row refers to optical position of the identified galaxy, in the following rows, the parameters refers to radio parameters -For A3432, the high flux 363.5mJy is likely an error (see "Post-Publication Notes" above) Remarks: A367: there is a very faint (2 sigma) radio source right at the position of the galaxy. A1791: the radio source is complex, and the galaxy is almost certainly associated with the source. A2854: there is little doubt that the dumbbell system and the radio source are associated, even though the positional coincidence is difficult to judge, due to the absence of a strong, well-defined radio core. A3150: there are three galaxies close to the radio source. This is the only unclear case in the whole sample. The identification should be considered uncertain. A3151: one galaxy falls right inside the double radio source, so the identification is probably correct. A3391: the radio source is complex; a faint core is present and lies close (~5 arcsec) to the eastern galaxy of the dumbbell system, and we therefore consider the radio source associated with this galaxy. A3432: see "Post-Publication Notes" A3532: similar to the case of A1791: one galaxy is in between the two lobes of a double source. The identification is quite likely correct. A3618: the western galaxy is probably the one associated with the radio source. A3706: the radio identification is uncertain due to the very faint radio source associated. -------------------------------------------------------------------------------- Historical Notes: *02-Mar-1994: first released *14-Oct-1994: ReadMe modified ================================================================================ (End) Patricia Bauer [CDS] 14-Oct-1994