Interaction-induced HI gas concentration with centrally-enhanced star formation in ALFALFA-SDSS galaxies
Yanhan Guo, Cheng Li

TL;DR
This study shows that galaxy interactions increase central HI gas concentration and star formation, with stronger effects in low-mass galaxies, highlighting the role of tidal forces in galaxy evolution.
Contribution
It provides a large-scale statistical analysis linking HI gas concentration and star formation enhancement to galaxy interactions, using the HI profile parameter $K$.
Findings
Higher HI concentration correlates with increased clustering and nearby neighbors.
Tidal interactions cause synchronized increases in gas concentration and star formation.
Central galaxies show stronger gas and star formation enhancements than satellites.
Abstract
We present a statistical analysis for the interaction-induced central concentration of HI gas distributions and its connection with interaction-induced central star formation enhancement, using a large sample of galaxies from the ALFALFA and SDSS surveys. By adopting the HI profile parameter , an indicator of gas concentration inferred from the integrated 21 cm emission line, we find that galaxies with more centrally concentrated HI (higher values) or enhanced specific star foramtion rate (sSFR) exhibit significantly stronger clustering and higher probability of hosting a nearby neighbor on scales below , which is more pronounced in low-mass galaxies. Furthermore, by utilizing the enhancement functions for a sample of galaxy pairs, we directly trace the evolution of HI concentration and sSFR enhancement as a function of projected separation. Our…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Astrophysics and Star Formation Studies
