Multiphase Astrophysics to Unveil the Virgo Environment (MAUVE)

Autor(en)

Barbara Catinella, Luca Cortese, Jiayi Sun, Toby Brown, Eric Emsellem, Amelia Fraser-McKelvie, Adam B. Watts, Amy Attwater, Andrew Battisti, Alessandro Boselli, Woorak Choi, Aeree Chung, Elisabete da Cunha, Sara Ellison, Pavel Jáchym, Maria J. Jimenez-Donaire, Tutku Kolcu, Bumhyun Lee, James McGregor, Ian Roberts, Eva Schinnerer, Kristine Spekkens, Sabine Thater, David Thilker, Jesse van de Sande, Vicente Villanueva, Thomas G. Williams, Nikki Zabel

Abstrakt

The Multiphase Astrophysics to Unveil the Virgo Environment (MAUVE) project is a multi-facility programme exploring how dense environments transform galaxies. Combining a VLT/MUSE P110 Large Programme and ALMA observations of 40 late-type Virgo Cluster galaxies, MAUVE resolves star formation, kinematics, and chemical enrichment within their molecular gas discs. A key goal is to track the evolution of cold gas that survives in the inner regions of satellites after entering the cluster, and how it evolves across different infall stages. With its high spatial resolution -- probing down to the physical scales of giant molecular cloud complexes -- and multiphase synergy, MAUVE aims to offer a time-resolved view of environmental quenching and set a new benchmark for cluster galaxy studies.

Organisation(en)

Institut für Astrophysik

Journal

The Messenger,

DOI

https://doi.org/10.18727/0722-6691/5393

Publikationsdatum

11-2025

ÖFOS 2012

103003 Astronomie, 103004 Astrophysik

Schlagwörter

Link zum Portal

https://ucrisportal.univie.ac.at/de/publications/c7aded84-4590-4d21-a837-3d752e1b74cf