J/ApJS/80/501 VLA survey of Abell clusters. II. (Owen+ 1992)
A 20 centimeter VLA survey of Abell clusters of galaxies.
II. Images and optical identifications
Owen F.N., White R.A., Burns J.O.
<Astrophys. J. Suppl. Ser. 80, 501 (1992)>
=1992ApJS...80..501O 1992ApJS...80..501O (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, galaxy ; Radio sources
Keywords: galaxies: active - galaxies: clustering - galaxies: jets -
radio continuum: galaxies - surveys
Abstract:
We present radio contour maps, models, and optical identifications for
130 radio galaxies in Abell clusters of galaxies.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1 66 144 Radio galaxy parameters
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See also:
VIII/29 : 1400-MHz Survey of 1478 Abell Galaxy Clusters (Owen+ 1982)
J/AJ/109/14 : Optical spectroscopy of Abell clusters. I. (Owen+ 1995)
J/AJ/98/64 : VLA survey of Abell clusters of galaxies I. (Zhao+ 1989)
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: table1
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Bytes Format Units Label Explanations
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1- 4 I4 --- Abell ? Abell cluster number (1)
5 A1 --- --- [-]
6 A1 --- m_Abell Multiplicity index on Abell number
8- 9 I2 h RAh Right ascension (1950.0)
11- 12 I2 min RAm Right ascension (1950.0)
14- 18 F5.2 s RAs Right ascension (1950.0)
20 A1 --- DE- Declination sign
21- 22 I2 deg DEd Declination (1950.0)
24- 25 I2 arcmin DEm Declination (1950.0)
27- 30 F4.1 arcsec DEs Declination (1950.0)
32- 35 F4.1 mag Rmag Estimate of the R magnitude of the galaxy
37- 41 I5 mJy Flux ? Total flux density of the associated
radio source (2)
43- 47 F5.2 arcsec MajAxis ? Major axis of the CLEAN beam of the
radio image used for the analysis
49- 53 F5.2 arcsec MinAxis ? Minor axis of the CLEAN beam of the
radio image used for the analysis
55- 60 F6.2 deg PA ? Position angle of the CLEAN beam of the
radio image used for the analysis
62- 66 A5 --- Ref References (3)
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Note (1): 1927-A : alternative identification is 14" SE of galaxy marked.
2306-A : Galaxy is at plate limit and does not reproduce well
in the glossy.
Note (2): If the column is blank, the galaxy listed is an alternate
identification for the last radio source with a flux density
listed about it.
Note (3): References
1: O'Donoghue A.A., Owen F.N., Eilek J.A., 1990ApJS...72...75O 1990ApJS...72...75O
2: Giovannini G., Feretti L., Gregorini L., 1987A&AS...69..171G 1987A&AS...69..171G
3: Gregorini L., Bondi M., 1989A&A...225..333G 1989A&A...225..333G
4: Taylor et al., 1990ApJ...360...41T 1990ApJ...360...41T
5: de Ruiter et al., 1986A&AS...65..111D 1986A&AS...65..111D
6: Fanti et al., 1987A&AS...69...57F 1987A&AS...69...57F
7: Zhao J.-H., Burns J.O., Owen F.N., 1989AJ.....98...64Z 1989AJ.....98...64Z
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History: Prepared via OCR at CDS.
References:
Zhao et al., Paper I. 1989AJ.....98...64Z 1989AJ.....98...64Z, Cat. J/AJ/98/64
Owen et al., Paper III. 1993ApJS...87..135O 1993ApJS...87..135O
Ledlow et al., Paper IV. 1995AJ....109..853L 1995AJ....109..853L, Cat. J/AJ/109/853
Ledlow et al., Paper V. 1995AJ....110.1959L 1995AJ....110.1959L, Cat. J/AJ/110/1959
Owen et al., Paper VII. 1997ApJS..108...41O 1997ApJS..108...41O
(End) James Marcout, Patricia Bauer [CDS] 15-Sep-1997