Bibcode
Barrena, R.; Boschin, W.; Girardi, M.; Spolaor, M.
Referencia bibliográfica
Astronomy and Astrophysics, Volume 467, Issue 1, May III 2007, pp.37-48
Fecha de publicación:
5
2007
Revista
Número de citas
31
Número de citas referidas
30
Descripción
Aims:To conduct an intensive study of the rich, X-ray luminous galaxy
cluster Abell 773 at z = 0.22 containing a diffuse radio halo to
determine its dynamical status. Methods: Our analysis is based on
new spectroscopic data obtained at the TNG telescope for 107 galaxies,
37 spectra recovered from the CFHT archive and new photometric data
obtained at the Isaac Newton Telescope. We use statistical tools to
select 100 cluster members (out to 1.8 h^-1_70 from the cluster
centre), to analyse the kinematics of cluster galaxies and to determine
the cluster structure. Our analysis is also performed by using X-ray
data stored in the Chandra archive. Results: The 2D distribution
shows two significant peaks separated by 2´ in the EW direction
with the main western one closely located at the position of the two
dominant galaxies and the X-ray peak. The velocity distribution of
cluster galaxies shows two peaks at v 65000 and 67500 km
s-1, corresponding to the velocities of the two dominant
galaxies. The low velocity structure has a high velocity dispersion -
σv = 800-1100 km s-1 - and its galaxies are
centred on the western 2D peak. The high velocity structure has
intermediate velocity dispersion - σv˜ 500 km
s-1 - and is characterized by a complex 2D structure with a
component centred on the western 2D peak and a component centred on the
eastern 2D peak, these components probably being two independent groups.
We estimate a cluster mass within 1h^-1_70 of 6-11h^-1_70 M_&sun;. Our
analysis of Chandra data shows the presence of two very close peaks in
the core and the elongation of the X-ray emission in the NEE-SWW
direction. Conclusions: Our results suggest we are looking at
probably two groups in an advanced stage of merging with a main cluster
and having an impact velocity Δ {{v}_rf} 2300 km s-1.
In particular, the radio halo seems to be related to the merger of the
eastern group.
Figures 1 and 2 are only available in electronic form at
http://www.aanda.org Table 1 is only available in electronic form at the
CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via
http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/467/37