A SALT Spectral Study of S0s Hosting Pseudobulges
Kaustubh Vaghmare, Sudhanshu Barway, Petri V\"ais\"anen, Rajin, Ramphul, Yogesh Wadadekar, and Ajit Kembhavi

TL;DR
This study uses SALT spectroscopy to analyze the star formation histories of S0 galaxies with pseudobulges, revealing diverse evolutionary processes influenced by bars and gas content.
Contribution
It provides detailed spectroscopic evidence of star formation and bar effects in S0 pseudobulges, expanding understanding of their formation and evolution.
Findings
Unbarred galaxies show extended star formation histories.
Presence of strong emission lines indicates active star formation.
Barred galaxies exhibit older stellar populations, suggesting accelerated formation.
Abstract
We present a SALT-RSS spectroscopic study of a sample of S0 galaxies established by Vaghmare et al. (2015) as having pseudobulges using a combination of photometric criteria. We extract the spectra of various regions along the galaxy major axis using standard long-slit spectroscopic reduction procedures and model the spectra using STARLIGHT to derive detailed star formation histories. The central spectra of galaxies without bars in our sample reveal a complex star formation history, which is consistent with the belief that pseudobulges have a history of star formation distributed over extended periods of time. The spectra of the unbarred galaxies contain strong emission lines such as H , indicating active star formation, which appears to be in contradiction with the expectation that S0 galaxies have been stripped of gas. In the case of the two barred galaxies in the sample, the…
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