Si ricorda che gli Associati INAF (Esterni, quali ad esempio personale universitario) NON devono confermare le proprie FTE. Gli associati hanno facoltà di leggere la scheda INAF nella parte pubblica senza necessità di account.
Scheda AGN feedback
FINAL
Scheda convalidata, con Checksum 707991af5d2db2d12bc0bff0fc8374e763bba358a3c97e5cf4ac2a2c5e998e62
Scheda madre delle seguenti Schede figlie
Titolo Scheda
Acronimo
Coordinatore
Azione
GTO ERIS per lo studio dell'evoluzioni delle galassie: AGN feedback e ISM evolution
L'obiettivo di questo programma è verificare se feedback da buchi neri (BN) e' il responsabile per il regolamento della crescita delle galassie massicce. Il programma sarà realizzato sfruttando due risorse principali: a) la grande quantità di dati dedicati raccolti sulla strumentazione di punta (MUSE, SINFONI e ALMA per mappare gas ionizzati e molecolari nelle galassie ospiti di AGN, XMM per sondare i venti nucleari); b) un team esperto e affiatato, che conta sia ricercatori orientati all'osservazione che modellisti. Alla fine del nostro progetto otterremo vincoli alla fisica del feedback da BN. Se questo feedback non fosse una soluzione praticabile, saremmo costretti a cercare un nuovo driver fisico per il regolamento della crescita delle galassie massicce.
The goal of this program is to assess or disprove black hole (BH) feedback as the physical driver for the quenching of massive galaxies. The program will be achieved exploiting two main assets: a) the large amount of dedicated data collected on today's flagship intrumentation (MUSE, SINFONI and ALMA to map ionized and molecular gas in AGN host galaxies, XMM to probe AGN nuclear winds); b) an experienced and close-knit team, counting both observation-oriented and model-oriented researchers. At the end of our project we would quantitatively assess BH feedback physics. Should BH feedback not be a viable solution, we would be forced to look for a new physical driver for the quenching of massive galaxies, probably an even more important result.
Galassie, AGN e loro evoluzione
Fisica degli oggetti compatti galattici ed extragalattici
15. Team Summary
15. Personale INAF coinvolto
Numero di partecipanti INAF al progetto: 28
Struttura
Nfte
N0
TI 2024
TI 2025
TI 2026
TD 2024
TD 2025
TD 2026
Nex
Extra
O.A. TRIESTE
6
0
0.50
0.50
0.40
0.90
0.70
0.30
0
0.00
IAPS ROMA
0
0
0.00
0.00
0.00
0.00
0.00
0.00
0
0.00
O.A. PADOVA
0
0
0.00
0.00
0.00
0
0
0
1
0.10
OAS BOLOGNA
0
0
0.00
0.00
0.00
0
0
0
0
0.00
O.A. ROMA
1
0
0.10
0.10
0.00
0
0
0
0
0.00
IASF MILANO
1
0
0.20
0.20
0.00
0
0
0
0
0.00
IRA BOLOGNA
0
0
0.00
0.00
0.00
0
0
0
0
0.00
O.A. ARCETRI
0
0
0.00
0.00
0.00
0
0
0
0
0.00
Totali
8
0
0.80
0.80
0.40
0.90
0.70
0.30
1
0.10
16. Personale Associato INAF coinvolto
Numero di partecipanti Associati INAF: 13
#
Struttura
TI 2024
TI 2025
TI 2026
TD 2024
TD 2025
TD 2026
Extra
1
Università di Bologna
0.10
0.10
0.10
0
0
0
0.00
2
Scuola Normale Superiore
0.00
0.00
0.00
0
0
0
0.00
3
Università degli Studi di Roma - Tor Vergata
0.00
0.00
0.00
0
0
0
0.00
4
Università Roma 3
0.00
0.00
0.00
0
0
0
0.00
5
Scuola Normale Superiore di Pisa
0.00
0.00
0.00
0
0
0
0.00
6
Universita' di Firenze
0.00
0.00
0.00
0
0
0
0.00
7
ASI
0.00
0.00
0.00
0
0
0
0.00
8
Università di Firenze
0
0
0
0.00
0.00
0.00
0.00
9
University of Ljubljana
0
0
0
0.20
0.20
0.20
0.00
10
Università Roma Tre
0.00
0.00
0.00
0
0
0
0.00
11
Dipartimento di Fisica, Università di Trieste, Sezione di Astronomia
0
0
0
0.20
0.20
0.20
0.00
12
SISSA
0
0
0
0.50
0.00
0.00
0.00
Totali
0.10
0.10
0.10
0.90
0.40
0.40
0.00
Fondi a sostegno
21. Totale fondi a disposizione (dato aggregato, k€)
Certi 2024
Certi 2025
Certi 2026
Presunti 2024
Presunti 2025
Presunti 2026
70729.0
70705.0
0.0
0.0
0.0
0.0
Produzione scientifica e tecnologica
22. Produzione scientifica e tecnologica - Highlights
#
DOI
Descrizione
Azione
1
10.1093/mnras/stz255
Titolo: The AGN fuelling/feedback cycle in nearby radio galaxies I. ALMA observations and early results
Autori:Ilaria Ruffa and Isabella Prandoni and Robert A Laing and Rosita Paladino and Paola Parma and Hans ....
Publisher:Oxford University Press (OUP)
Rivista: Monthly Notices of the Royal Astronomical Society
Anno pubblicazione:2019
2
10.3847/1538-4357/ab1a3a
Titolo: Outflows in the Disks of Active Galaxies
Autori:N. Menci and F. Fiore and C. Feruglio and A. Lamastra and F. Shankar and E. Piconcelli and E. Giall ....
Publisher:American Astronomical Society
Rivista: The Astrophysical Journal
Anno pubblicazione:2019
3
https://doi.org/10.1051/0004-6361/201937292
Titolo: The WISSH quasars project
Autori:L. Zappacosta and E. Piconcelli and M. Giustini and G. Vietri and F. Duras and G. Miniutti and M. B ....
Publisher:EDP Sciences
Rivista: Astronomy \& Astrophysics
Anno pubblicazione:2020
4
10.3847/1538-4357/ab67bd
Titolo: Multiphase Gas Flows in the Nearby Seyfert Galaxy ESO428\textendashG014. Paper I
Autori:C. Feruglio and G. Fabbiano and M. Bischetti and M. Elvis and A. Travascio and F. Fiore
Publisher:American Astronomical Society
Rivista: The Astrophysical Journal
Anno pubblicazione:2020
5
10.1051/0004-6361/201936197
Titolo: The WISSH quasars project
Autori:A. Travascio and L. Zappacosta and S. Cantalupo and E. Piconcelli and F. Arrigoni Battaia and M. Gi ....
Publisher:EDP Sciences
Rivista: Astronomy \& Astrophysics
Anno pubblicazione:2020
6
10.1093/mnras/stz2410
Titolo: Constraints on high-J CO emission lines in z $\sim$ 6 quasars
Autori:S Carniani and S Gallerani and L Vallini and A Pallottini and M Tazzari and A Ferrara and R Maiolin ....
Publisher:Oxford University Press (OUP)
Rivista: Monthly Notices of the Royal Astronomical Society
Anno pubblicazione:2019
7
10.1051/0004-6361/201834372
Titolo: The MAGNUM survey: different gas properties in the outflowing and disc components in nearby active galaxies with MUSE
Autori:M. Mingozzi and G. Cresci and G. Venturi and A. Marconi and F. Mannucci and M. Perna and F. Belfior ....
Publisher:EDP Sciences
Rivista: Astronomy \& Astrophysics
Anno pubblicazione:2019
8
10.1051/0004-6361/202039057
Titolo: The WISSH quasars project
Autori:M. Bischetti and C. Feruglio and E. Piconcelli and F. Duras and M. P\'erez-Torres and R. Herrer ....
Publisher:EDP Sciences
Rivista: Astronomy \& Astrophysics
Anno pubblicazione:2021
We study the impact of active galactic nuclei (AGN) ionised outflows on star formation in high-redshift AGN host galaxies, by combining near-infrared integral field spectroscopic (IFS) observations, mapping the Hα emission and [O III]λ5007 outflows, with matched-resolution observations of the rest-frame far-infrared (FIR) emission. We present high-resolution ALMA Band 7 observations of eight X-ray selected AGN (L2 − 10 keV = 1043.8 − 1045.2 erg s−1) at z ∼ 2 from the SUPER (SINFONI Survey for Unveiling the Physics and Effect of Radiative feedback) sample, targeting the observed-frame 870 μm (rest-frame ∼260 μm) continuum at ∼2 kpc (0.2″) spatial resolution. The targets were selected among the SUPER AGN with an [O III] detection in the IFS maps and with a detection in the FIR photometry. We detected six out of eight targets with signal-to-noise ratio S/N ≳ 10 in the ALMA maps, from which we measured continuum flux densities in the range 0.27 − 2.58 mJy and FIR half-light radii (Re) in the range 0.8 − 2.1 kpc. The other two targets were detected with S/N of 3.6 and 5.9, which are insufficient for spatially resolved analysis. The FIR Re of our sample are comparable to other AGN and star-forming galaxies at a similar redshift from the literature. However, combining our sample with the literature samples, we find that the mean FIR size in X-ray AGN (Re = 1.16 ± 0.11 kpc) is slightly smaller than in non-AGN (Re = 1.69 ± 0.13 kpc). From spectral energy distribution fitting, we find that the main contribution to the 260 μm flux density is dust heated by star formation, with ≤4% contribution from AGN-heated dust and ≤1% from synchrotron emission. The majority of our sample show different morphologies for the FIR (mostly due to reprocessed stellar emission) and the ionised gas emission (Hα and [O III], mostly due to AGN emission). This could be due to the different locations of dust and ionised gas, the different sources of the emission (stars and AGN), or the effect of dust obscuration. We are unable to identify any residual Hα emission, above that dominated by AGN, that could be attributed to star formation. Under the assumption that the FIR emission is a reliable tracer of obscured star formation, we find that the obscured star formation activity in these AGN host galaxies is not clearly affected by the ionised outflows. However, we cannot rule out that star formation suppression is happening on smaller spatial scales than the ones we probe with our observations (< 2 kpc) or on different timescales.
9
10.1038/s41586-022-04608-1
Suppression of black-hole growth by strong outflows at redshifts 5.8-6.6, Bischetti et al. 2022, Nature