Photometric study of the IC 65 group of galaxies
J. Vennik, U. Hopp

TL;DR
This study conducts a comprehensive photometric analysis of the IC 65 galaxy group, identifying new dwarf members, examining interaction effects, and assessing the group's evolutionary stage using multi-wavelength data.
Contribution
It introduces new photometric data for dwarf galaxy members and provides insights into the group's early dynamical evolution and interaction effects.
Findings
Four probable dwarf members identified with new photometric parameters
Presence of H II regions indicating active star formation in dwarf galaxies
Evidence of mild interactions and early-stage evolution in the group
Abstract
We carry out a photometric study of a poor group of late-type galaxies around IC 65, with the aim: (a) to search for new dwarf members and to measure their photometric characteristics; (b) to search for possible effects of mutual interactions on the morphology and star-formation characteristics of luminous and faint group members; (c) to evaluate the evolutionary status of this particular group. We make use of our BRI CCD observations, DPOSS blue and red frames, and the 2MASS JHK frames. In addition, we use the HI imaging data, the far-infrared and radio data from the literature. Search for dwarf galaxies is made using the SExtractor software. Detailed surface photometry is performed with the MIDAS package. Four LSB galaxies were classified as probable dwarf members of the group and the BRI physical and model parameters were derived for the first time for all true and probable group…
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