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A MUSE inquiry into the physical processes taking place within the Abell 2667 Brightest Cluster Galaxy

Published online by Cambridge University Press:  10 June 2020

E. Iani Open the ORCID record for E. Iani [Opens in a new window] ,
G. Rodighiero ,
J. Fritz ,
G. Cresci ,
C. Mancini ,
P. Tozzi ,
L. Rodríguez-Muñoz ,
P. Rosati ,
G. B. Caminha  and
S. Berta
...Show all authors
E. Iani
Affiliation:
Dipartimento di Fisica ed Astronomia, Università degli Studi di Padova, Vicolo dell’Osservatorio 3, I-35122 Padova, Italy email: [email protected] European Southern Observatory, Karl Schwarzschild Straß e 2, D-85748 Garching, Germany
G. Rodighiero
Affiliation:
Dipartimento di Fisica ed Astronomia, Università degli Studi di Padova, Vicolo dell’Osservatorio 3, I-35122 Padova, Italy email: [email protected] INAF - Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, I-35122 Padova, Italy
J. Fritz
Affiliation:
Instituto de Radioastronomía y Astrofísica, UNAM, Campus Morelia, A.P. 3-72, C.P. 58089, Mexico
G. Cresci
Affiliation:
INAF - Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, I-50125 Firenze, Italy
C. Mancini
Affiliation:
Dipartimento di Fisica ed Astronomia, Università degli Studi di Padova, Vicolo dell’Osservatorio 3, I-35122 Padova, Italy email: [email protected] INAF - Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, I-35122 Padova, Italy
P. Tozzi
Affiliation:
INAF - Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, I-50125 Firenze, Italy
L. Rodríguez-Muñoz
Affiliation:
Dipartimento di Fisica ed Astronomia, Università degli Studi di Padova, Vicolo dell’Osservatorio 3, I-35122 Padova, Italy email: [email protected]
P. Rosati
Affiliation:
Dipartimento di Fisica e Scienze della Terra, Università degli Studi di Ferrara, Via Saragat 1, I-44122 Ferrara, Italy
G. B. Caminha
Affiliation:
Kapteyn Astronomical Institute, University of Groningen, Postbus 800, 9700 AV Groningen, The Netherland
S. Berta
Affiliation:
Institut de Radioastronomie Millimétrique 300 rue de la Piscine, Domaine Universitaire 38406 Saint Martin d’Hères, France
P. Cassata
Affiliation:
Dipartimento di Fisica ed Astronomia, Università degli Studi di Padova, Vicolo dell’Osservatorio 3, I-35122 Padova, Italy email: [email protected]
A. Concas
Affiliation:
Excellence Cluster Universe, Boltzmannstraß e 2, D-85748 Garching, Germany
A. Enia
Affiliation:
Dipartimento di Fisica ed Astronomia, Università degli Studi di Padova, Vicolo dell’Osservatorio 3, I-35122 Padova, Italy email: [email protected]
D. Fadda
Affiliation:
SOFIA Science Center, USRA, NASA Ames Research Center, M.S. N232-12 Moffett Field, CA 9403
A. Franceschini
Affiliation:
Dipartimento di Fisica ed Astronomia, Università degli Studi di Padova, Vicolo dell’Osservatorio 3, I-35122 Padova, Italy email: [email protected]
A. Liu
Affiliation:
INAF - Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, I-50125 Firenze, Italy
A. Mercurio
Affiliation:
INAF - Osservatorio Astronomico di Capodimonte, via Moiariello 16, 80131 Napoli, Italy
L. Morselli
Affiliation:
Excellence Cluster Universe, Boltzmannstraß e 2, D-85748 Garching, Germany
P. G. Pérez-González
Affiliation:
Departamento de Astronomía y Astrofísica, Universidad Complutense de Madrid, Av. Complutense s/n, C.P. 28040, Madrid, Spain Centro de Astrobiologa (CAB, INTA-CSIC), Carretera de Ajalvir km 4, E-28850 Torrejón de Ardoz, Madrid, Spain
P. Popesso
Affiliation:
Excellence Cluster Universe, Boltzmannstraß e 2, D-85748 Garching, Germany
G. Sabatini
Affiliation:
Dipartimento di Fisica e Astronomia, Università degli Studi di Bologna, via Gobetti 93/2, I-40129 Bologna, Italy INAF - Istituto di Radioastronomia - Italian node of the ALMA Regional Centre (ARC), via Gobetti 101, I-40129 Bologna, Italy
A. Zanella
Affiliation:
European Southern Observatory, Karl Schwarzschild Straß e 2, D-85748 Garching, Germany
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Abstract

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Brightest cluster galaxies (BCGs) residing in cool-core clusters are known to be the stage of intricate baryon cycle phenomena (e.g. gas inflows, AGN outflows, star formation feedback). The scenarios describing the observed properties of these galaxies are still controversial, suffering from limitations due to the spatial resolving power of the instruments, specifically for galaxies beyond the Local Universe. However, the dramatic improvements introduced by the integral-field unit instruments (e.g. MUSE) could shed light on the physical processes driving the evolution of these galaxies. We present an extensive analysis of the stellar and gas properties (i.e. kinematics, stellar mass, star formation rate) of the radio-loud BCG sitting at the centre of the X-ray luminous cool-core cluster Abell 2667 (z = 0.23), based on MUSE data. Our results indicate that the BCG is a massive elliptical, hosting an AGN that is possibly undergoing accretion of cold star-forming clouds of ICM or galactic cannibalism.

Keywords

galaxies: elliptical and lenticular, cDgalaxies: evolutiongalaxies: kinematics and dynamicsgalaxies: nuclei(galaxies:) cooling flows
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S341: Challenges in Panchromatic Modelling with Next Generation Facilities , November 2019 , pp. 83 - 87
Copyright
© International Astronomical Union 2020

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