Table 3.
Groups and clusters which are members of the Local SC.
| Name | RA | Dec | Redshift | FX | Error | LX | m200 | rout | nH | Alt. name |
|---|---|---|---|---|---|---|---|---|---|---|
| RXCJ1226.2+1257 | 186.5540 | 12.9577 | 0.0033 (a) | 34.2216 | 3.80 | 0.0166 | 0.295 | 17.5 | 2.6 | M86 |
| RXCJ1230.7+1223 | 187.6838 | 12.3915 | 0.0033 | 371.7451 | 1.20 | 0.1792 | 1.291 | 17.5 | 2.5 | M87 (Virgo) |
| RXCJ1242.8+0241 | 190.7098 | 2.6884 | 0.0031 | 16.6059 | 8.50 | 0.0112 | 0.231 | 10.5 | 1.8 | NGC 4636 |
| RXCJ1501.1+0141 | 225.2994 | 1.6981 | 0.0061 | 13.1537 | 6.30 | 0.0267 | 0.396 | 8.5 | 4.2 | NGC 5813 |
| RXCJ1506.4+0136 | 226.6237 | 1.6022 | 0.0062 | 8.2915 | 13.80 | 0.0111 | 0.230 | 13.0 | 4.3 | NGC 5846 |
Notes. The flux, FX, is in units of 10−12 erg s−1 cm−2 in the 0.1–2.4 keV band and the error in the following column is in per cent. The X-ray luminosity, LX, is in units of 1044 erg s−1 at 0.1 to 2.4 keV within r500, m200 is the cluster mass estimated from the LX-mass relation within r200, rout is the radius in arcmin out to which the X-ray luminosity is detected in the RASS, and nH is the interstellar column density in the line-of-sight in units of 1020 cm−2. In the last column we designate groups by the name of the central dominant galaxy.
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