Multiphase Astrophysics to Unveil the Virgo Environment (MAUVE)

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

doi:10.18727/0722-6691/5393

Multiphase Astrophysics to Unveil the Virgo Environment (MAUVE)

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

Institut für Astrophysik

Veröffentlichungen: Beitrag in Fachzeitschrift › Artikel › Peer Reviewed

Abstract

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.

Originalsprache	Englisch
Seiten (von - bis)	15-18
Seitenumfang	4
Fachzeitschrift	The Messenger
Jahrgang	195
DOIs	https://doi.org/10.18727/0722-6691/5393
Publikationsstatus	Veröffentlicht - 1 Sept. 2025

ÖFOS 2012

103003 Astronomie
103004 Astrophysik

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10.18727/0722-6691/5393Lizenz: CC BY 4.0

Zitationsweisen

Catinella, B., Cortese, L., Sun, J., Brown, T., Emsellem, E., Fraser-McKelvie, A., Watts, A. B., Attwater, A., Battisti, A., Boselli, A., Choi, W., Chung, A., da Cunha, E., Ellison, S., Jáchym, P., Jimenez-Donaire, M. J., Kolcu, T., Lee, B., McGregor, J., ... Zabel, N. (2025). Multiphase Astrophysics to Unveil the Virgo Environment (MAUVE). The Messenger, 195, 15-18. https://doi.org/10.18727/0722-6691/5393

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title = "Multiphase Astrophysics to Unveil the Virgo Environment (MAUVE)",

abstract = "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. ",

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

note = "Copyright European Southern Observatory",

year = "2025",

month = sep,

day = "1",

doi = "10.18727/0722-6691/5393",

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Catinella, B, Cortese, L, Sun, J, Brown, T, Emsellem, E, Fraser-McKelvie, A, Watts, AB, Attwater, A, Battisti, A, Boselli, A, Choi, W, Chung, A, da Cunha, E, Ellison, S, Jáchym, P, Jimenez-Donaire, MJ, Kolcu, T, Lee, B, McGregor, J, Roberts, I, Schinnerer, E, Spekkens, K, Thater, S, Thilker, D, van de Sande, J, Villanueva, V, Williams, TG & Zabel, N 2025, 'Multiphase Astrophysics to Unveil the Virgo Environment (MAUVE)', The Messenger, Jg. 195, S. 15-18. https://doi.org/10.18727/0722-6691/5393

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AU - Catinella, Barbara

AU - Cortese, Luca

AU - Sun, Jiayi

AU - Brown, Toby

AU - Emsellem, Eric

AU - Fraser-McKelvie, Amelia

AU - Watts, Adam B.

AU - Attwater, Amy

AU - Battisti, Andrew

AU - Boselli, Alessandro

AU - Choi, Woorak

AU - Chung, Aeree

AU - da Cunha, Elisabete

AU - Ellison, Sara

AU - Jáchym, Pavel

AU - Jimenez-Donaire, Maria J.

AU - Kolcu, Tutku

AU - Lee, Bumhyun

AU - McGregor, James

AU - Roberts, Ian

AU - Schinnerer, Eva

AU - Spekkens, Kristine

AU - Thater, Sabine

AU - Thilker, David

AU - van de Sande, Jesse

AU - Villanueva, Vicente

AU - Williams, Thomas G.

AU - Zabel, Nikki

N1 - Copyright European Southern Observatory

PY - 2025/9/1

Y1 - 2025/9/1

N2 - 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.

AB - 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.

KW - astro-ph.GA

U2 - 10.18727/0722-6691/5393

DO - 10.18727/0722-6691/5393

M3 - Article

VL - 195

SP - 15

EP - 18

JO - The Messenger

JF - The Messenger

ER -

Multiphase Astrophysics to Unveil the Virgo Environment (MAUVE)

Abstract

ÖFOS 2012

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Zitationsweisen