Fetching the paper…
Reading the bibliography…
It has been recently shown that the observed morphological properties of the Bullet Cluster can be accurately reproduced in hydrodynamical simulations only when the infall pairwise velocity V_{c} of the system exceeds 3000km/s (or at least possibly 2500 km/s) at the pair separation of 2R_{vir}, where R_{vir} is the virial radius of the main cluster, and that the probability of finding such a bullet-like system is extremely low in the standard \Lambda CDM cosmology.
Nothing clear enough to list yet.
Nothing clear enough to list yet.
Nothing clear enough to list yet.
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…