J/AJ/118/625        Radio sources in Abell 2125 and 2645    (Dwarakanath+, 1999)

On the different radio source populations in the Butcher-Oemler clusters Abell 2125 and 2645. Dwarakanath K.S., Owen F.N. <Astron. J. 118, 625 (1999)> =1999AJ....118..625D 1999AJ....118..625D (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, galaxy ; Radio sources Keywords: galaxies: clusters: individual (Abell 2125, Abell 2645) - galaxies: starburst - radio continuum Abstract: The Abell clusters 2125 and 2645 have different radio source populations, despite being very similar in richness (Abell class 4) and redshift (0.25). The number density of radio sources in Abell 2125 is almost an order of magnitude more than that in Abell 2645, based on observations to the same optical and radio luminosities of the two clusters. About 30% of the radio sources in Abell 2125 shows signs of star formation, with the largest concentration of them in the southwest clump 2Mpc from the cluster center. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 61 54 Abell 2125: optical identifications table3.dat 61 36 Abell 2645: optical identifications -------------------------------------------------------------------------------- Table 1: Relevant cluster and observational parameters -------------------------------------------------------------------------------- Cluster z N30 fB Field center VLA Beam PA rms RA (2000) DE " deg uJy/beam -------------------------------------------------------------------------------- Abell 2125 0.2460 62 0.19 15 41.0 +66 18.5 C 13.7 x 11.5 -7.4 25 15 41.2 +66 16. A 1.83 x 1.73 -48.4 ∼30 Abell 2645 0.2500 35 0.03 23 41.6 -09 01.4 B 5.33 x 4.15 +2.2 27 Abell 370 0.373 107 0.21 02 36.5 -01 34.9 B 5.22 x 4.25 +23.1 12 Cl 0024+1654 0.391 87 0.16 00 26.6 +17 10.6 B 4.53 x 4.32 +23.8 10 -------------------------------------------------------------------------------- Notes: N30 is a measure of cluster richness. It indicates 30% of the total number of cluster members brighter than MV=-20. fB, the fraction of blue galaxies in a cluster, s the fraction of the total net cluster population with rest-frame B-V colors at least 0.2mag bluer than those of the early-type galaxies (Butcher & Oemler, 1984ApJ...285..426B 1984ApJ...285..426B). VLA configurations A, B, and C have maximum baselines of approximately 35, 11, and 3 km, respectively. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- [DO99] Sequential number (1) 4- 5 I2 h RAh Radio right ascension (J2000.0) 7- 8 I2 min RAm Radio right ascension (J2000.0) 10- 14 F5.2 s RAs Radio right ascension (J2000.0) 16 A1 --- DE- Radio declination sign (J2000.0) 17- 18 I2 deg DEd Radio declination (J2000.0) 20- 21 I2 arcmin DEm Radio declination (J2000.0) 23- 26 F4.1 arcsec DEs Radio declination (J2000.0) 28- 31 F4.2 arcsec Sep Radial distance between the optical and radio positions 33- 36 F4.1 arcsec Ext1 ? Extent (as measured in the radio image) 38- 41 F4.1 arcsec Ext2 ? Extent (as measured in the radio image) 43- 45 I3 deg PA ? Position angle 47 A1 --- Memb [Y/N] Member? 49 A1 --- StarFor [Y/N] Star formation? 51- 55 I5 uJy S20cm Flux density at 20cm 57- 61 F5.1 10+22W/Hz L20cm ? Luminosity at 20cm (2) -------------------------------------------------------------------------------- Note (1): Designation in Simbad: Table2: [DO99] ACO 2125 NN in Simbad Table3: [DO99] ACO 2645 NN in Simbad Note (2): The luminosities are in the observer's rest frame and are estimated using z=0.2460, H0=75km/s/Mpc, and q_0-=0.1. -------------------------------------------------------------------------------- History: From AJ electronic version
(End) James Marcout, Patricia Bauer [CDS] 21-Oct-1999
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