LX-σ relation of galaxy clusters (Shen+, 2008)

Details LX-σ relation of galaxy clusters (Shen+, 2008) LX-σ relation of galaxy clusters (Shen+, 2008)

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..73891074s&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/389/1074. Originally published in: 2008MNRAS.389.1074S

Physics

Clusters: Galaxy, X-Ray Sources, Velocity Dispersion

Scientific paper

We use the RASS to study the X-ray properties of our sample of groups and clusters. The RASS mapped the sky in the soft X-ray band (0.1-2.4keV) with exposure time varying between 400 and 40000s, depending on direction on the sky. The resolution of the RASS images is 45 arcsec.
(1 data file).

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