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Table 1

Properties of the different Virgo cluster substructures.

Substructure RA Dec Dist Ref. < vel > σ Ref. R200 M200 Ref. ρICM TICM Ref. Central
J2000 J2000 Mpc km s−1 km s−1 Mpc M× 1014 cm−3 keV
Cluster A 187.71 12.39 16.5 1, 2 955 799 3 1.55 1.4–4.2 4–9 2.0 × 10−3 2.3 10, 11 M87
Cluster B 187.44 8.00 23 1 1134 464 3 0.96 1 9 M49
Cluster C 190.85 11.45 16.5 1 1073 545 3 0.66–1.15 0.35–1.85 12, 13 M60
W cloud 185.00 5.80 32 1 2176 416 3 0.50–0.88 0.15–0.83 12, 13 NGC4261
W′ cloud 186.00 7.20 23 1 1019 416 3 0.50–0.88 0.15–0.83 12, 13 NGC4365
M cloud 183.00 13.40 32 1 2109 280 3 0.34–0.60 0.05–0.26 12, 13 NGC4168
LVC cloud 184.00 13.40 16.5 1 85 208 3 0.25–0.44 0.02–0.11 12, 13 NGC4216

References. (1) Gavazzi et al. (1999); (2) Mei et al. (2007); (3) Boselli et al. (2014a,b,c); (4) Nulsen & Böhringer (1995); (5) Girardi et al. (1998); (6) Schindler et al. (1999); (7) McLaughlin (1999); (8) Urban et al. (2011); (9) Ferrarese et al. (2012); (10) Böhringer (2005), priv. comm.; (11) Böhringer et al. (1994); (12) derived using the M200 vs. σ relation given in Biviano et al. (2006); (13) derived using the M200 vs. σ relation given in Evrard et al. (2008).

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