Bubbles and outflows: The novel JWST/NIRSpec view of the <i>z</i>=1.59 obscured quasar XID2028

Simple item page
dc.contributor.authorCresci, G.
dc.contributor.authorTozzi, G.
dc.contributor.authorPerna, M.
dc.contributor.authorBrusa, M.
dc.contributor.authorMarconcini, C.
dc.contributor.authorMarconi, A.
dc.contributor.authorCarniani, S.
dc.contributor.authorBrienza, M.
dc.contributor.authorGiroletti, M.
dc.contributor.authorBelfiore, F.
dc.contributor.authorGinolfi, M.
dc.contributor.authorMannucci, F.
dc.contributor.authorUlivi, L.
dc.contributor.authorScholtz, J.
dc.contributor.authorVenturi, G.
dc.contributor.authorArribas, S.
dc.contributor.authorUbler, H.
dc.contributor.authorD'Eugenio, F.
dc.contributor.authorMingozzi, M.
dc.contributor.authorBalmaverde, B.
dc.contributor.authorCapetti, A.
dc.contributor.authorParlanti, E.
dc.contributor.authorZana, T.
dc.date.accessioned2025-01-20T20:15:17Z
dc.date.available2025-01-20T20:15:17Z
dc.date.issued2023
dc.description.abstractQuasar feedback in the form of powerful outflows is invoked as a key mechanism to quench star formation in galaxies, although direct observational evidence is still scarce and debated. Here we present Early Release Science JWST NIRSpec IFU observations of the z = 1.59 prototypical obscured Active Galactic Nucleus (AGN) XID2028: This target represents a unique test case for studying quasar feedback at the peak epoch of AGN-galaxy co-evolution because extensive multi-wavelength coverage is available and a massive and extended outflow is detected in the ionised and molecular components. With the unprecedented sensitivity and spatial resolution of the JWST, the NIRSpec dataset reveals a wealth of structures in the ionised gas kinematics and morphology that were previously hidden in the seeing-limited ground-based data. In particular, we find evidence of an interaction between the interstellar medium of the galaxy and the quasar-driven outflow and radio jet that produces an expanding bubble from which the fast and extended wind detected in previous observations emerges. The new observations confirm the complex interplay between the AGN jet, wind and the interstellar medium of the host galaxy, highlighting the role of low-luminosity radio jets in AGN feedback. They also clearly show the new window that NIRSpec opens for detailed studies of feedback at high redshift.
dc.fuente.origenWOS
dc.identifier.doi10.1051/0004-6361/202346001
dc.identifier.eissn1432-0746
dc.identifier.issn0004-6361
dc.identifier.urihttps://doi.org/10.1051/0004-6361/202346001
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/92251
dc.identifier.wosidWOS:000967616600014
dc.language.isoen
dc.revistaAstronomy & astrophysics
dc.rightsacceso restringido
dc.subjectgalaxies: active
dc.subjectgalaxies: jets
dc.subjectgalaxies: individual: XID2028
dc.subjectISM: jets and outflows
dc.subjecttechniques: imaging spectroscopy
dc.titleBubbles and outflows: The novel JWST/NIRSpec view of the <i>z</i>=1.59 obscured quasar XID2028
dc.typeartículo
dc.volumen672
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
Files
Collections
Artículos de revistas