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arXiv · astro-ph/0610116

Small Scale Systems of Galaxies. III. X-ray detected E+S galaxy pairs in low density environments

R. Gruetzbauch·G. Trinchieri·R. Rampazzo·E. V. Held·L. Rizzi·J. W. Sulentic·W. W. Zeilinger
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Abstract

We present a comprehensive study of the local environments of four E+S galaxy pairs with the main goal to investigate their formation/evolution histories. New XMM-Newton data were obtained for two pairs (RR 143 and RR 242) that complements existing ROSAT data for the other two (RR 210 and RR 216). The new observations reveal diffuse X-ray emission in both pairs. The emission is asymmetric in both cases and extends out to 120 kpc and 160 kpc in RR 143 and RR 242 respectively. The nucleus of RR 242 hosts a low luminosity mildly absorbed AGN. We find that the early-type components of pairs with diffuse hot gas appear to be relaxed objects while those in RR 210 and RR 216, where no diffuse emission has been found, display unambiguous signatures of ongoing interaction. Wide-field V and R-band data are used to study the photometric properties of the early-type components and to search for a candidate faint galaxy populations around each of the pairs. While no diffuse optical light is found for any of the pairs, all of the early-type members show very extended and concentric luminous envelopes. We identify a faint galaxy sample in each field and we consider whether they could be physically associated with the luminous pairs based upon (V-R) colors and photometric properties. We find that the distribution of r_e and M_R for the candidates are similar in three of the fields (RR 143, 216 and 242). The same selection criteria applied to the field of RR 210 suggest a fainter and more compact population possibly suggesting a larger background fraction than in the other fields.

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R. Gruetzbauch, G. Trinchieri, R. Rampazzo, E. V. Held, L. Rizzi, J. W. Sulentic, W. W. Zeilinger. 2006-10-04. Small Scale Systems of Galaxies. III. X-ray detected E+S galaxy pairs in low density environments. https://doi.org/10.1086/509657

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