J/A+A/338/813       Galaxy clusters σ-T relationship (Wu+ 1998)

Updating the σ-T relationship for galaxy clusters Wu X.-P., Fang L.-Z., Xu W. <Astron. Astrophys. 338, 813 (1998)> =1998A&A...338..813W 1998A&A...338..813W (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, galaxy ; Velocity dispersion Keywords: galaxies: clusters: general - X-rays: galaxies Description: This is a sample of 149 galaxy clusters for which both the X-ray determined temperature T of the intracluster gas and the optical measured velocity dispersion σ of the cluster galaxies have been available. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 57 149 Cluster Sample table1.ps 72 854 PostScript version of table1.dat table1.tex 76 284 LaTeX version of table1.dat -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- Cluster Cluster name 13- 18 F6.4 --- z Redshift 20- 24 F5.2 keV T Temperature of the X-ray intracluster gas 26- 29 F4.2 keV E_T ? Error in T (upper limit) 31- 34 F4.2 keV e_T ? Error in T (lower limit) 36- 39 I4 km/s sigma Velicoty dispersion of the cluster galaxies 41- 43 I3 km/s E_sigma ? Error in sigma (upper limit) 45- 47 I3 km/s e_sigma ? Error in sigma (lower limit) 49- 52 F4.2 --- beta β spectral index 54- 57 F4.2 --- e_beta ? rms uncertainty on beta -------------------------------------------------------------------------------- Acknowledgements: Xiang-Ping Wu ,
(End) Patricia Bauer [CDS] 14-Aug-1998
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