From spirals to lenticulars: evidence from the rotation curves and mass models of three early-type galaxies
Alexandra V. Shelest, Federico Lelli

TL;DR
This study derives rotation curves for three lenticular galaxies, revealing similarities with late-type galaxies in mass distribution and dark matter properties, suggesting recent transition from spiral to early-type without major structural changes.
Contribution
First detailed rotation curve analysis of ETGs combining CO and HI data, showing their dark matter halos and stellar mass-to-light ratios are similar to those of LTGs.
Findings
ETGs have rotation curves similar to LTGs of comparable mass.
Stellar mass-to-light ratios in ETGs are low and comparable to star-forming LTGs.
Dark matter halos follow LTG scaling relations.
Abstract
Rotation curves have traditionally been difficult to trace for early-type galaxies (ETGs) because they often lack a high-density disk of cold gas as in late-type galaxies (LTGs). We derive rotation curves for three lenticular galaxies from the ATLAS3D survey, combining CO data in the inner parts with deep HI data in the outer regions, extending out to 10-20 effective radii. We also use Spitzer photometry at 3.6 um to decompose the rotation curves into the contributions of baryons and dark matter (DM). We find that (1) the rotation-curve shapes of these ETGs are similar to those of LTGs of similar mass and surface brightness; (2) the dynamicallyinferred stellar mass-to-light ratios are small for quiescent ETGs but similar to those of star-forming LTGs; (3) the DM halos follow the same scaling relations with galaxy luminosity as those of LTGs; (4) one galaxy (NGC 3626) is poorly fitted…
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