📝 SummarXiv

Abstract

Context: In dense environments, disk galaxies can be subjected to tidal interactions with other galaxies and/or ram pressure stripping. Some morphological features are clearly associated with one or the other interaction (e.g. tidal bridges vs long one-sided linear gas tails). But, under certain circumstances, both mechanisms can result in morphological features that could be confused, such as lopsided or asymmetric disks and unwinding spiral arms. Aims: Our aim is to develop new measures for application to asymmetric galaxies of this type that distinguish gravitational-only tidal interactions from ram pressure stripping, and that can be applied directly to simulations, and potentially to observations. Methods: We define a new measure for galaxies called the Size-Shape Difference (SSD) measure. This measure is sensitive to differences in the size and shape of a younger stellar population (<200 Myr) compared to that of an intermediate age stellar population (200-400 Myr). We use numerical simulations of galaxies undergoing gravitational-only tidal interactions and/or undergoing ram pressure stripping to test the measure. Results: Because ram pressure tends to directly alter the gas distribution, the younger stellar population (which best traces out the gas distribution) tends to change shape and morphology with respect to the intermediate age population. The SSD measure is sensitive to this change, and we find it can effectively distinguish between ram pressure and gravitational-only tidal encounters. In fact, we find it is even more effective when a combination of a tidal interaction and ram pressure has occurred together, as may arise in dense environments. As tidal interactions tend to enhance the spiral structure in disk galaxies, the effectiveness of the SSD measure is further enhanced when combined with a measure of the strength of the spiral arms.