Marco Baldi
Marco Baldi
Marco Baldi
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This result is in stark contrast with previous claims, which found the<br />
opposite behavior for the density profiles of CDM halos<br />
! / ! crit<br />
MB et al., 0812.3901 (MNRAS 2010)<br />
10 5<br />
10 4<br />
10 3<br />
10 2<br />
10 1<br />
Tuesday, July 6, 2010<br />
Resuts (IV): halo density profiles<br />
Halo Density profiles for CDM and baryons for Group nr. 0<br />
"CDM<br />
RP1<br />
RP2<br />
RP5<br />
M200("CDM) = 2.82510e+14 h -1 M O•<br />
10 100 1000<br />
R (h -1 kpc)<br />
<strong>Marco</strong> <strong>Baldi</strong> - MGADS, Strasbourg 16 VI 2010<br />
Macciò et al., 2004
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