Per una genealogia della giustizia penale internazionale: ambiguita' e paradossi

This article aims to consider the role for a critical criminology outside the national dimension, highlighting its continuities with studies in the critical tradition which have suggested the need to address State criminality and criminogenic structures more in general, but also suggesting a critique of international criminal law as a governmentality project.It reconstructs the genealogy of the international criminal justice system, following on from Schmitt and other well known authors, but it focuses in specific on its paradoxes, contradictions and ambiguities rather than its purely political effect. The authors argue that critical criminologists should engage with the international dimension of crime and control and approach this venture of a international criminal justice system as the possibility of “telling the truth” about State atrocities without missing on using strategically the category of human rights and law to bring to the fore minoritarian interests which are
usually denied by power discourses and economic forces.

SN 2004aw: confirming diversity of Type Ic supernovae

Optical and near-infrared (near-IR) observations of the Type Ic supernova (SN Ic) 2004aw are presented, obtained from -3 to +413 d with respect to the B-band maximum. The photometric evolution is characterized by a comparatively slow post-maximum decline of the light curves. The peaks in redder bands are significantly delayed relative to the bluer bands, the I-band maximum occurring 8.4 d later than that in B. With an absolute peak magnitude of -18.02 in the V band the SN can be considered fairly bright, but not exceptional. This also holds for the U through I bolometric light curve, where SN 2004aw has a position intermediate between SNe 2002ap and 1998bw. Spectroscopically SN 2004aw provides a link between a normal SN Ic like SN 1994I and the group of broad-lined SNe Ic. The spectral evolution is rather slow, with a spectrum at day +64 being still predominantly photospheric. The shape of the nebular [O-I] lambda lambda 6300, 6364 line indicates a highly aspherical explosion. Helium cannot be unambiguously identified in the spectra, even in the near-IR. Using an analytical description of the light-curve peak we find that the total mass of the ejecta in SN 2004aw is 3.5-8.0 M-circle dot, significantly larger than that in SN 1994I, although not as large as in SN 1998bw. The same model suggests that about 0.3 M-circle dot of Ni-56 has been synthesized in the explosion. No connection to a GRB can be firmly established.