Molecular Gas and Star Formation in Local Early-Type Galaxies
M. Bureau, T. A. Davis, K. Alatalo, A. F. Crocker, L. Blitz, L. M., Young, F. Combes, M. Bois, F. Bournaud, M. Cappellari, R. L. Davies, P. T. de, Zeeuw, P.-A. Duc, E. Emsellem, S. Khochfar, D. Krajnovic, H. Kuntschner,, P.-Y. Lablanche, R. M. McDermid, R. Morganti, T. Naab

TL;DR
This study investigates molecular gas presence and star formation in local early-type galaxies, revealing diverse gas morphologies, external origins, and atypical star formation behaviors, challenging traditional galaxy evolution models.
Contribution
First complete large CO survey of local early-type galaxies, revealing high detection rates and diverse gas morphologies, with implications for galaxy evolution.
Findings
22% detection rate of molecular gas in early-type galaxies
External origin of gas in over a third of systems
Early-type galaxies show diverse star formation behaviors
Abstract
The molecular gas content of local early-type galaxies is constrained and discussed in relation to their evolution. First, as part of the Atlas3D survey, we present the first complete, large (260 objects), volume-limited single-dish survey of CO in normal local early-type galaxies. We find a surprisingly high detection rate of 22%, independent of luminosity and at best weakly dependent on environment. Second, the extent of the molecular gas is constrained with CO synthesis imaging, and a variety of morphologies is revealed. The kinematics of the molecular gas and stars are often misaligned, implying an external gas origin in over a third of the systems, although this behaviour is drastically diffferent between field and cluster environments. Third, many objects appear to be in the process of forming regular kpc-size decoupled disks, and a star formation sequence can be sketched by…
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