The complex structure of Abell 2345: a galaxy cluster with non-symmetric radio relics

Home

All issues

Volume 521 (October 2010)

A&A, 521 (2010) A78

Full HTML

Free Access

Table 3:

Kinematical properties of cluster and subclumps.
Analysis	System	$N_{\rm g}$	$\langle v\rangle$	$\sigma_{V}$
			${\rm km\ s^{-1}}$	${\rm km\ s^{-1}}$
	A2345	98	$53\,645\pm108$	$\rm 1069_{-62}^{+75}$
1D DEDICA	low vel. peak^a	53	53202	>604
1D DEDICA	high vel. peak^a	45	54142	>538
${\rm {<}0.3}\,h_{70}^{-1}\,{\rm Mpc}$	${\rm E{-}clump}$	18	$54\,573\pm232$	$\rm 944_{-297}^{+303}$
${\rm {<}0.3}\,h_{70}^{-1}\,{\rm Mpc}$	${\rm SW{-}clump}$	8	$53\,995\pm540$	$\rm 1346_{-102}^{+289}$
${\rm {<}0.3}\,h_{70}^{-1}\,{\rm Mpc}$	${\rm NW{-}clump}$	9	$53\,487\pm407$	$\rm 1105_{-122}^{+182}$
3D KMM	${\rm E{-}clump}$	52	$53\,908\pm162$	$\rm 1155_{-70}^{+119}$
${\rm 3D}\,{\rm KMM}$	${\rm SW{-}clump}$	17	$53\,517\pm261$	$\rm 1032_{-106}^{+218}$
3D KMM	${\rm NW{-}clump}$	29	$53\,312\pm166$	$\rm 873_{-91}^{+167}$
${\rm 3D}\,{\rm KMM}\,{\rm (}r{\rm ^{\prime}<20)}$	${\rm E{-}clump}$	45	$54\,077\pm170$	$\rm 1128_{-89}^{+123}$
${\rm 3D}\,{\rm KMM}\,{\rm (}r{\rm ^{\prime}<20)}$	${\rm SW{-}clump}$	13	$53\,079\pm244$	$\rm 831_{-110}^{+217}$
${\rm 3D}\,{\rm KMM}\,{\rm (}r{\rm ^{\prime}<20)}$	${\rm NW{-}clump}$	30	$53\,296\pm159$	$\rm 852_{-74}^{+165}$

Notes. ^aFor this galaxy clump we report the velocity peak instead on the mean velocity. The value of velocity dispersion should be considered a minor limit due to the abruptal truncation of the velocity distribution.

Source LaTeX | All tables | In the text

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.