A mid-IR study of Hickson compact groups - II. Multiwavelength analysis of the complete GALEX-Spitzer sample

T. Bitsakis; V. Charmandaris; E. da Cunha; T. Díaz-Santos; E. Le Floc’h; G. Magdis

doi:doi:10.1051/0004-6361/201117355

Issue		A&A Volume 533, September 2011


Article Number		A142
Number of page(s)		29
Section		Extragalactic astronomy
DOI		http://dx.doi.org/10.1051/0004-6361/201117355
Published online		16 September 2011

Online material

Table 4

The morphological type and derived physical parameters based on the SED modeling of the HCG galaxies.

Table 4

continued.

Table 5

Derived physical parameters based on the SED modeling of the interacting pair’s galaxy sample.

Table 6

Distance to, virial radius, and morphology of the nearest neighbor, as well as “strength” of interaction for the HCG galaxies.

Table 6

continued.

Table 7

Observed and predicted 60 μm and 100 μm IRAS fluxes for each group, as well as total HI, H₂, stellar, and dynamical masses.

© ESO, 2011

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