Search catalogue
J/AJ/98/64 VLA survey of Abell clusters of galaxies I. (Zhao+ 1989)
A 20cm VLA survey of Abell clusters of galaxies. I. Distance class <3 clusters. Zhao J.-H., Burns J.O., Owen F.N. <Astron. J. 98, 64 (1989)> =1989AJ.....98...64Z
ADC_Keywords: Clusters, galaxy ; Radio sources ; X-ray sources Abstract: We report the results of a VLA survey at 20cm of a complete sample of nearby Abell clusters (D≤3). We have compiled an extensive catalog of cluster radio sources with S20>10mJy from a combination of our VLA observations and observations of similar resolution with the Westerbork Synthesis Radio Telescope (WSRT). Using these radio data and X-ray data from the Einstein observatory, we have analyzed the properties of these clusters. Unlike that previously suggested, no significant correlation is found between 20cm radio power and X-ray luminosity. There is weak evidence that richer clusters have a higher probability of radio emission. Based on Rood-Sastry morphological types of clusters, we do not find any strong evidence that regular-type clusters are statistically more likely to be radio loud than irregular-type clusters. However, Bautz-Morgan types I and II-III are found to have comparable radio-detection rates; but Bautz-Morgan Type III clusters are likely to have a lower radio-detection rate. A weak correlation between X-ray-cooling mass-accretion rates and radio powers was found for central, dominant galaxies in cooling-flow clusters. This might suggest that either cooling accretion directly fuels the central engine and/or cooling flows strongly interact with (e.g., confine) the radio plasma. In addition, radio sources associated with central dominant galaxies in cooling-flow clusters tend to be small in comparison with those in non-cooling-flow clusters. This might suggest that cooling flows tend to obstruct the propagation of radio jets from central, dominant galaxies. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file cluster.dat 175 110 *Abell cluster properties (from table4) radio.dat 220 166 *Abell cluster radio sources (from table4) optical.dat 87 178 *Optical identifications of the radio sources refs.dat 106 79 References notes.dat 97 37 Notes on clusters
Note on cluster.dat, radio.dat and optical.dat: the 3 files are the data contained in table4 "Radio sources and X-ray data of Abell clusters (D≤3)".
See also: VII/110 : Rich Clusters of Galaxies (Abell+ 1989) J/ApJS/80/501 : VLA survey of Abell clusters. II. (Owen+ 1992) J/AJ/109/853 : VLA survey of Abell clusters. IV. (Ledlow+ 1995) J/AJ/110/1959 : VLA survey of Abell clusters. V. (Ledlow+ 1995) Byte-by-byte Description of file: cluster.dat
Bytes Format Units Label Explanations
1 A1 --- --- [A] 2- 5 I4 --- Abell Abell (Cat. VII/110) Cluster Number 7- 8 I2 h RAh Right ascension (1950) 10- 13 F4.1 min RAm Right ascension (1950) 15 A1 --- DE- Declination sign (1950) 16- 17 I2 deg DEd Declination (1950) 19- 20 I2 arcmin DEm Declination (1950) 22- 25 F4.1 mag m10 Magnitude of the tenth-brightness galaxy 27 I1 --- Class [0/2] Richness classification 29- 33 F5.4 --- z ? Redshift 35- 45 A11 ---- BM Bautz-Morgan type 47- 50 A4 --- RS Rood-Sastry (1971PASP...83..313R) type 52- 54 I3 --- NA Number of galaxies in the cluster 56- 89 A34 --- MT Hubble morphological type 91 A1 --- l_LX Limit flag on LX 92- 99 E8.3 10-7W LX ? X-ray luminosity 100 A1 --- n_LX [abwW] Note on LX (1) 103 A1 --- l_RX Limit flag on RX 104-107 F4.3 Mpc RX ? Core radius of the X-ray region (lower limit if interval) 108 A1 --- n_RX [-] -: when interval 109-111 F3.2 Mpc RX2 ? Upper limit of RX when interval 113 A1 --- l_No Limit flag on No 114-120 E7.2 cm-3 No ? Central gas density 122 A1 --- l_Mx Limit flag on Mx 123-129 E7.1 solMass Mx ? Intracluster mass 132-139 E8.2 yr tc ? Cluster cooling time 141-148 E8.1 yr e_tc ? rms uncertainty on tc 150 A1 --- l_LeX [≲] Limit flag on LeX 151-154 F4.1 % LeX ? Central X-ray luminosity excess 155 A1 --- n_LeX [-] -: when interval 156-157 I2 % LeX2 ? Upper limit of LeX when interval
Note (1): the symbols have the following meaning: w = within 0.67Mpc W = weak, within 0.33Mpc a = within 0.33Mpc b = within 0.67Mpc of center
Byte-by-byte Description of file: radio.dat
Bytes Format Units Label Explanations
1 A1 --- --- [A] 2- 5 I4 --- Abell Abell (Cat. VII/110) Cluster Number 7 I1 --- Nr Radiosource number in the cluster (1) 9- 15 F7.1 mJy S20cm Radiosource flux density at 1.5GHz (20cm) 17- 31 A15 --- MType Radiosource morphological type (2) 33 A1 --- l_Size Limit flag on size 34- 38 F5.1 arcsec Size ? Largest angular size of the radiosource 40- 41 I2 h RAh Right ascension (1950) 43- 44 I2 min RAm Right ascension (1950) 46- 50 F5.2 s RAs Right ascension (1950) 52 A1 --- DE- Declination sign (1950) 53- 54 I2 deg DEd Declination (1950) 56- 57 I2 arcmin DEm Declination (1950) 59- 63 F5.2 arcsec DEs Declination (1950) 65- 69 F5.3 --- D Ratio of the separation between the radio source and the cluster center to the Abell cluster radius 70 A1 --- n_D [*] *: the radiosource is outside 0.5 of the Abell cluster radius 72- 79 E8.2 W/Hz P20cm Radio power at 1.5GHz (20cm) 81-107 A27 --- Names Other names 108-127 A20 --- Ref Comma-separated list of reference numbers detailed in file "refs.dat"
Note (1): [ZBO89] ACO NNNN-N in Simbad Note (2): Abbreviations used: CP: compact NAT: narrow-angle tailed WAT: wide-angle tailed DB: double source UNK: unknown
Byte-by-byte Description of file: optical.dat
Bytes Format Units Label Explanations
1 A1 --- --- [A] 2- 5 I4 --- Abell Abell (Cat. VII/110) Cluster Number 7 I1 --- Nr Radiosource number in the cluster 9- 14 F6.5 --- z ? Redshift of optically identified galaxy 16- 17 I2 h RAh Right ascension (1950) 19- 20 I2 min RAm Right ascension (1950) 22- 26 F5.2 s RAs Right ascension (1950) 28 A1 --- DE- Declination sign (1950) 29- 30 I2 deg DEd Declination (1950) 32- 33 I2 arcmin DEm Declination (1950) 35- 39 F5.2 arcsec DEs Declination (1950) 41 A1 --- l_mag Limit flag on mag 42- 45 F4.1 mag mag ? Visual or photographic magnitude of the galaxy 46 A1 --- n_mag [bvp] Type of magnitude: v: V magnitude p: photographic magnitude b: b magnitude 48- 69 A22 --- MType Morphological type of the optically identified galaxy 71- 87 A17 --- Note Note
Byte-by-byte Description of file: refs.dat
Bytes Format Units Label Explanations
1- 2 I2 --- Ref Reference number 4- 22 A19 --- BibCode BibCode 24- 44 A21 --- Author Author names 46-106 A61 --- Com Comments
Byte-by-byte Description of file: notes.dat
Bytes Format Units Label Explanations
1 A1 --- --- [A] 2- 5 I4 --- Abell Abell (Cat. VII/110) Cluster Number 7- 97 A91 --- Note Text of the note
History: Prepared via OCR at CDS; proof-read and corrected by H. Andernach () on 5-Nov-2004. References: Owen et al., Paper II. 1992ApJS...80..501O, Cat. J/ApJS/80/501 Owen et al., Paper III. 1993ApJS...87..135O Ledlow et al., Paper IV. 1995AJ....109..853L, Cat. J/AJ/109/853 Ledlow et al., Paper V. 1995AJ....110.1959L, Cat. J/AJ/110/1959 Owen & Ledlow, Paper VII. 1997ApJS..108...41O
(End) James Marcout, Patricia Vannier [CDS] (Jan-1999) H. Andernach 05-Nov-2004
| The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line |
© UDS/CNRS