Formation of S0s in extreme environments III: the role of environment in the formation pathways
Lodovico Coccato (1), Amelia Fraser-McKelvie (2,3), Yara L. Jaff\'e, (4), Evelyn J. Johnston (5), Arianna Cortesi (6,7), Diego Pallero (4) ((1), European Southern Observatory, Karl-Schwarzchild-str.,2, 85748 Garching b. M, unchen, Germany

TL;DR
This study investigates how different environments influence the formation pathways of S0 galaxies, finding that the faded spiral scenario dominates in denser environments while mergers are more common in less dense regions.
Contribution
It combines kinematic, morphological, and stellar population data from 329 S0 galaxies to link formation pathways with environmental conditions.
Findings
Faded spiral pathway is more efficient in dense environments.
Merger pathway is more prevalent in low-density regions.
Environmental density influences the dominant formation mechanism.
Abstract
It is well established that there are at least two main channels to form lenticular (or S0) galaxies. The first, which we name "faded spiral" scenario, includes quenching events that led to consumption or removal of gas from a spiral progenitor. The second, which we call "merger" scenario, includes merger-like events and interactions between galaxies. Each scenario leaves characteristic signatures in the newly-formed lenticular galaxy. However, the conditions that trigger one mechanism over another are still unknown. This paper is the third of a series aimed at understanding the role of the environment in the formation of lenticular galaxies. In this study, we combine the kinematics, morphology, and properties of the stellar populations of 329 S0s from the SAMI and MaNGA surveys in order to highlight the role of the environment in the process.We divide the S0s into two classes (A and B)…
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