
Example of high-resolution re-simulations.
The upper-left panel shows the projection of a region of 30 Mpc/
side around a massive (
M
) dark matter halo,
obtained in the VLS cosmological N-body simulations carried out by the Virgo
Consortium (Yoshida et al. 2001).
The upper-right panel is a zoom in the 2 r
(
Mpc/
)
region centered on the main halo; the mass resolution is
M
, and about
particles are shown in the image.
The lower panels are the corresponding images in the high-resolution
re-simulations: the mass resolution is now
M
, and more than
particles are contained within the virial
radius of the re-simulated halo. Credit: B. Lanzoni, G. Tormen, V. Springel,
G. Mamon, S.D. White.
People involved at OAB:
Observational extragalactic astronomy has traditionally been one of
the main themes of research at the Bologna Observatory. It includes
a wide range of subjects, from the structure and evolution of ``normal"
galaxies, to the physical properties of active galactic nuclei
(AGNs) to observational cosmology.
The extragalactic research at the Bologna Observatory is characterized
by a multiwavelength approach: while optical astronomy is the main field
at the Observatory, some of the scientific staff
specialize in X-ray observations of AGNs, and others find their main
interest in radio studies of galaxies and quasars.
Much of this research is based on an intensive use of the most advanced
instruments available today: the X-ray satellites Chandra and
XMM-Newton, the ESO optical/NIR telescopes (including VLT), the
Westerbork, VLA and ATCA radiotelescopes.