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J/A+AS/101/475      Spectroscopic observations of A3571 (Quintana+, 1993)

Spectroscopic observations of the galaxy cluster A 3571 (SC 1344-325) Quintana H., de Souza R. <Astron. Astrophys. Suppl. Ser. 101, 475 (1993)> =1993A&AS..101..475Q (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, galaxy ; Radial velocities Keywords: clusters of galaxies - X-ray clusters - galaxies velocities Abstract: Spectroscopic data and density counts are presented for this southern cluster, which seems to belong to the outskirts of the Shapley 8 concentration (= A 3558 = SC 1326-311). Using telescopes at the Cerro Tololo Interamerican Observatory and La Silla Observatory a total of 72 galaxy velocities were measured giving a mean redshift of 0.0384 and a global velocity dispersion of 1022 (+99, -77) km/s. A preliminary analysis of velocity and density data suggests the presence of various subgroups. The central core of the cluster is dominated by a very elongated, distorded and diffuse cD galaxy. This cluster may be an example where the cD was formed early in the collapse process of a cluster which has not reached overall virialization yet. The derived X-ray luminosity of ∼2x1044erg/s in the 2-6keV band places this cluster in the group of strong X-ray cluster sources. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1 68 72 Galaxy velocities in SC 1344-325 = A 3571
Byte-by-byte Description of file: table1
Bytes Format Units Label Explanations
1- 3 I3 --- Name Object name 6- 7 I2 h RAh Right ascension (1950) 9- 10 I2 min RAm Right ascension (1950) 12- 15 F4.1 s RAs Right ascension (1950) 17 A1 --- DE- Declination sign 18- 19 I2 deg DEd Declination (1950) 21- 22 I2 arcmin DEm Declination (1950) 24- 25 I2 arcsec DEs Declination (1950) 28- 32 I5 km/s HV Heliocentic velocity 34- 35 I2 --- Nline ? Number of lines measured in each spectrum 37- 42 A6 --- Qual Quality comment 44- 49 A6 --- Tel Telescope (1) 51- 54 A4 --- Group Subclustering group 56- 68 A13 --- Note Notes
Note (1): 3.6OPT: OPTOPUS T1IT: CTIO 1m E1IT: ESO 1.5m T4V: CTIO 4m
History: OCR by LEDA team (Lyon Observatory) for the name, position and velocity columns, proof-read by H. Andernach in December 1994 (LEDA ref no. 24257). The other columns were added at CDS.
(End) Patricia Bauer [CDS] 18-Nov-1997
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

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