Widespread AGN feedback in a forming brightest cluster galaxy at z = 4.1, unveiled by JWST

We present rest-frame optical JWST Near-infrared Spectrograph (NIRSpec) integral field unit (IFU) spectroscopy of TN J1338−1942 at z = 4.1, one of the most luminous galaxies in the early universe with powerful extended radio jets. Previous observations showed evidence for strong, large-scale outflow...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Saxena, Aayush (VerfasserIn) , Overzier, Roderik A (VerfasserIn) , Villar-Martín, Montserrat (VerfasserIn) , Heckman, Tim (VerfasserIn) , Roy, Namrata (VerfasserIn) , Duncan, Kenneth J (VerfasserIn) , Röttgering, Huub (VerfasserIn) , Miley, George (VerfasserIn) , Aydar, Catarina (VerfasserIn) , Best, Philip (VerfasserIn) , Bosman, Sarah (VerfasserIn) , Cameron, Alex J (VerfasserIn) , Gabányi, Krisztina Éva (VerfasserIn) , Humphrey, Andrew (VerfasserIn) , Morais, Sandy (VerfasserIn) , Onoue, Masafusa (VerfasserIn) , Pentericci, Laura (VerfasserIn) , Reynaldi, Victoria (VerfasserIn) , Venemans, Bram (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: July 2024
In: Monthly notices of the Royal Astronomical Society
Year: 2024, Jahrgang: 531, Heft: 4, Pages: 4391-4407
ISSN:1365-2966
DOI:10.1093/mnras/stae1406
Online-Zugang:Verlag, kostenfrei, Volltext: https://doi.org/10.1093/mnras/stae1406
Volltext
Verfasserangaben:Aayush Saxena, Roderik A. Overzier, Montserrat Villar-Martín, Tim Heckman, Namrata Roy, Kenneth J. Duncan, Huub Röttgering, George Miley, Catarina Aydar, Philip Best, Sarah E.I. Bosman, Alex J. Cameron, Krisztina Éva Gabányi, Andrew Humphrey, Sandy Morais, Masafusa Onoue, Laura Pentericci, Victoria Reynaldi, Bram Venemans

MARC

LEADER 00000caa a2200000 c 4500
001 1910464309
003 DE-627
005 20250716213425.0
007 cr uuu---uuuuu
008 241202s2024 xx |||||o 00| ||eng c
024 7 |a 10.1093/mnras/stae1406  |2 doi 
035 |a (DE-627)1910464309 
035 |a (DE-599)KXP1910464309 
035 |a (OCoLC)1528014454 
040 |a DE-627  |b ger  |c DE-627  |e rda 
041 |a eng 
084 |a 29  |2 sdnb 
100 1 |a Saxena, Aayush  |e VerfasserIn  |0 (DE-588)1350003344  |0 (DE-627)1910508519  |4 aut 
245 1 0 |a Widespread AGN feedback in a forming brightest cluster galaxy at z = 4.1, unveiled by JWST  |c Aayush Saxena, Roderik A. Overzier, Montserrat Villar-Martín, Tim Heckman, Namrata Roy, Kenneth J. Duncan, Huub Röttgering, George Miley, Catarina Aydar, Philip Best, Sarah E.I. Bosman, Alex J. Cameron, Krisztina Éva Gabányi, Andrew Humphrey, Sandy Morais, Masafusa Onoue, Laura Pentericci, Victoria Reynaldi, Bram Venemans 
264 1 |c July 2024 
300 |b Illustrationen 
300 |a 17 
336 |a Text  |b txt  |2 rdacontent 
337 |a Computermedien  |b c  |2 rdamedia 
338 |a Online-Ressource  |b cr  |2 rdacarrier 
500 |a Veröffentlicht: 5. Juni 2024 
500 |a Gesehen am 02.12.2024 
520 |a We present rest-frame optical JWST Near-infrared Spectrograph (NIRSpec) integral field unit (IFU) spectroscopy of TN J1338−1942 at z = 4.1, one of the most luminous galaxies in the early universe with powerful extended radio jets. Previous observations showed evidence for strong, large-scale outflows based on its large (∼150 kpc) halo detected in Ly α, and high-velocity [O ii] emission features detected in ground-based spectroscopy. Our NIRSpec/IFU observations spatially resolve the emission line properties across the host galaxy. We find at least five concentrations of strong line emission, coinciding with discrete continuum features previously detected in imaging from Hubble Space Telescope and JWST, over an extent of ∼2 arcsec (∼15 kpc). The spectral diagnostics unambiguously trace active galactic nuclei (AGN) activity plus interaction between the interstellar medium and the radio jet as the dominant mechanisms for the ionization state and kinematics of the gas in the system. A secondary region of very high ionization lies at roughly 5 kpc away from the nucleus, and within the context of an expanding cocoon enveloping the radio lobe, this may be explained by strong shock-ionization of the entrained gas. However, it could also signal the presence of a second obscured AGN, which may offer an explanation for an intriguing outflow feature seen perpendicular to the radio axis. The presence of a dual supermassive black holes system in this galaxy would support that large galaxies in the early Universe quickly accumulated their mass through the merging of smaller units, at the centres of large overdensities. The inferred black hole mass to stellar mass ratio of 0.01−0.1 for TNJ1338 points to a more rapid assembly of black holes compared to the stellar mass of galaxies at high redshifts, consistent with other recent observations. 
700 1 |a Overzier, Roderik A  |e VerfasserIn  |4 aut 
700 1 |a Villar-Martín, Montserrat  |e VerfasserIn  |4 aut 
700 1 |a Heckman, Tim  |e VerfasserIn  |4 aut 
700 1 |a Roy, Namrata  |e VerfasserIn  |4 aut 
700 1 |a Duncan, Kenneth J  |e VerfasserIn  |4 aut 
700 1 |a Röttgering, Huub  |e VerfasserIn  |4 aut 
700 1 |a Miley, George  |e VerfasserIn  |4 aut 
700 1 |a Aydar, Catarina  |e VerfasserIn  |4 aut 
700 1 |a Best, Philip  |e VerfasserIn  |4 aut 
700 1 |a Bosman, Sarah  |e VerfasserIn  |0 (DE-588)1297436172  |0 (DE-627)185378124X  |4 aut 
700 1 |a Cameron, Alex J  |e VerfasserIn  |4 aut 
700 1 |a Gabányi, Krisztina Éva  |e VerfasserIn  |4 aut 
700 1 |a Humphrey, Andrew  |e VerfasserIn  |4 aut 
700 1 |a Morais, Sandy  |e VerfasserIn  |4 aut 
700 1 |a Onoue, Masafusa  |e VerfasserIn  |4 aut 
700 1 |a Pentericci, Laura  |e VerfasserIn  |4 aut 
700 1 |a Reynaldi, Victoria  |e VerfasserIn  |4 aut 
700 1 |a Venemans, Bram  |e VerfasserIn  |4 aut 
773 0 8 |i Enthalten in  |a Royal Astronomical Society  |t Monthly notices of the Royal Astronomical Society  |d Oxford : Oxford Univ. Press, 1827  |g 531(2024), 4 vom: Juli, Seite 4391-4407  |h Online-Ressource  |w (DE-627)314059164  |w (DE-600)2016084-7  |w (DE-576)090955420  |x 1365-2966  |7 nnas 
773 1 8 |g volume:531  |g year:2024  |g number:4  |g month:07  |g pages:4391-4407  |g extent:17  |a Widespread AGN feedback in a forming brightest cluster galaxy at z = 4.1, unveiled by JWST 
856 4 0 |u https://doi.org/10.1093/mnras/stae1406  |x Verlag  |x Resolving-System  |z kostenfrei  |3 Volltext 
951 |a AR 
992 |a 20241202 
993 |a Article 
994 |a 2024 
998 |g 1297436172  |a Bosman, Sarah  |m 1297436172:Bosman, Sarah  |d 130000  |d 130300  |e 130000PB1297436172  |e 130300PB1297436172  |k 0/130000/  |k 1/130000/130300/  |p 11 
999 |a KXP-PPN1910464309  |e 462951029X 
BIB |a Y 
SER |a journal 
JSO |a {"note":["Veröffentlicht: 5. Juni 2024","Gesehen am 02.12.2024"],"title":[{"title":"Widespread AGN feedback in a forming brightest cluster galaxy at z = 4.1, unveiled by JWST","title_sort":"Widespread AGN feedback in a forming brightest cluster galaxy at z = 4.1, unveiled by JWST"}],"person":[{"role":"aut","display":"Saxena, Aayush","family":"Saxena","given":"Aayush"},{"display":"Overzier, Roderik A","given":"Roderik A","family":"Overzier","role":"aut"},{"display":"Villar-Martín, Montserrat","given":"Montserrat","family":"Villar-Martín","role":"aut"},{"display":"Heckman, Tim","family":"Heckman","given":"Tim","role":"aut"},{"role":"aut","display":"Roy, Namrata","family":"Roy","given":"Namrata"},{"role":"aut","display":"Duncan, Kenneth J","given":"Kenneth J","family":"Duncan"},{"given":"Huub","family":"Röttgering","display":"Röttgering, Huub","role":"aut"},{"role":"aut","family":"Miley","given":"George","display":"Miley, George"},{"role":"aut","display":"Aydar, Catarina","given":"Catarina","family":"Aydar"},{"role":"aut","display":"Best, Philip","family":"Best","given":"Philip"},{"family":"Bosman","given":"Sarah","display":"Bosman, Sarah","role":"aut"},{"display":"Cameron, Alex J","given":"Alex J","family":"Cameron","role":"aut"},{"role":"aut","display":"Gabányi, Krisztina Éva","family":"Gabányi","given":"Krisztina Éva"},{"role":"aut","display":"Humphrey, Andrew","family":"Humphrey","given":"Andrew"},{"given":"Sandy","family":"Morais","display":"Morais, Sandy","role":"aut"},{"role":"aut","display":"Onoue, Masafusa","given":"Masafusa","family":"Onoue"},{"display":"Pentericci, Laura","given":"Laura","family":"Pentericci","role":"aut"},{"display":"Reynaldi, Victoria","family":"Reynaldi","given":"Victoria","role":"aut"},{"given":"Bram","family":"Venemans","display":"Venemans, Bram","role":"aut"}],"type":{"media":"Online-Ressource","bibl":"article-journal"},"origin":[{"dateIssuedKey":"2024","dateIssuedDisp":"July 2024"}],"physDesc":[{"extent":"17 S.","noteIll":"Illustrationen"}],"language":["eng"],"id":{"doi":["10.1093/mnras/stae1406"],"eki":["1910464309"]},"recId":"1910464309","name":{"displayForm":["Aayush Saxena, Roderik A. Overzier, Montserrat Villar-Martín, Tim Heckman, Namrata Roy, Kenneth J. Duncan, Huub Röttgering, George Miley, Catarina Aydar, Philip Best, Sarah E.I. Bosman, Alex J. Cameron, Krisztina Éva Gabányi, Andrew Humphrey, Sandy Morais, Masafusa Onoue, Laura Pentericci, Victoria Reynaldi, Bram Venemans"]},"relHost":[{"origin":[{"dateIssuedKey":"1827","publisherPlace":"Oxford ; Oxford [u.a.] ; Oxford [u.a.]","dateIssuedDisp":"1827-","publisher":"Oxford Univ. Press ; Blackwell ; Wiley-Blackwell"}],"type":{"media":"Online-Ressource","bibl":"periodical"},"pubHistory":["1.1827 -"],"title":[{"title_sort":"Monthly notices of the Royal Astronomical Society","title":"Monthly notices of the Royal Astronomical Society"}],"note":["Gesehen am 15.01.2018"],"recId":"314059164","id":{"eki":["314059164"],"issn":["1365-2966"],"zdb":["2016084-7"],"doi":["10.1111/(ISSN)1365-2966"]},"language":["eng"],"corporate":[{"display":"Royal Astronomical Society","role":"aut"}],"part":{"year":"2024","issue":"4","text":"531(2024), 4 vom: Juli, Seite 4391-4407","volume":"531","pages":"4391-4407","extent":"17"},"physDesc":[{"extent":"Online-Ressource"}],"disp":"Royal Astronomical SocietyMonthly notices of the Royal Astronomical Society"}]} 
SRT |a SAXENAAAYUWIDESPREAD2024