_version_ 1866913934458486784
author Onoue, Masafusa
Ding, Xuheng
Silverman, John D.
Matsuoka, Yoshiki
Izumi, Takuma
Strauss, Michael A.
Ward, Charlotte
Phillips, Camryn L.
Ito, Kei
Andika, Irham T.
Aoki, Kentaro
Arita, Junya
Baba, Shunsuke
Bieri, Rebekka
Bosman, Sarah E. I.
Eilers, Anna-Christina
Fujimoto, Seiji
Habouzit, Melanie
Haiman, Zoltan
Imanishi, Masatoshi
Inayoshi, Kohei
Iwasawa, Kazushi
Jahnke, Knud
Kashikawa, Nobunari
Kawaguchi, Toshihiro
Kohno, Kotaro
Lee, Chien-Hsiu
Li, Junyao
Lupi, Alessandro
Lyu, Jianwei
Nagao, Tohru
Overzier, Roderik
Schindler, Jan-Torge
Schramm, Malte
Scoggins, Matthew T.
Shimasaku, Kazuhiro
Toba, Yoshiki
Trakhtenbrot, Benny
Trebitsch, Maxime
Treu, Tommaso
Umehata, Hideki
Venemans, Bram
Vestergaard, Marianne
Volonteri, Marta
Walter, Fabian
Wang, Feige
Yang, Jinyi
Zhang, Haowen
author_facet Onoue, Masafusa
Ding, Xuheng
Silverman, John D.
Matsuoka, Yoshiki
Izumi, Takuma
Strauss, Michael A.
Ward, Charlotte
Phillips, Camryn L.
Ito, Kei
Andika, Irham T.
Aoki, Kentaro
Arita, Junya
Baba, Shunsuke
Bieri, Rebekka
Bosman, Sarah E. I.
Eilers, Anna-Christina
Fujimoto, Seiji
Habouzit, Melanie
Haiman, Zoltan
Imanishi, Masatoshi
Inayoshi, Kohei
Iwasawa, Kazushi
Jahnke, Knud
Kashikawa, Nobunari
Kawaguchi, Toshihiro
Kohno, Kotaro
Lee, Chien-Hsiu
Li, Junyao
Lupi, Alessandro
Lyu, Jianwei
Nagao, Tohru
Overzier, Roderik
Schindler, Jan-Torge
Schramm, Malte
Scoggins, Matthew T.
Shimasaku, Kazuhiro
Toba, Yoshiki
Trakhtenbrot, Benny
Trebitsch, Maxime
Treu, Tommaso
Umehata, Hideki
Venemans, Bram
Vestergaard, Marianne
Volonteri, Marta
Walter, Fabian
Wang, Feige
Yang, Jinyi
Zhang, Haowen
contents Understanding the rapid formation of supermassive black holes (SMBHs) in the early universe requires insight into stellar mass growth in host galaxies. Here, we present NIRSpec rest-frame optical spectra and NIRCam imaging from JWST of two galaxies at z>6, both hosting moderate-luminosity quasars. These galaxies exhibit Balmer absorption lines, similar to low-redshift post-starburst galaxies. Our analyses of the medium-resolution spectra and multiband photometry show bulk of the stellar mass (log (M_* / M_sun) > 10.6) formed in starburst episodes at redshift 9 and 7. One of the galaxies shows a clear Balmer break and lacks spatially resolved H alpha emission. It falls well below the star formation main sequence at z = 6, indicating quiescence. The other is transitioning to quiescence; together, these massive galaxies are among the most distant post-starburst systems known. The blueshifted wings of the quasar [O III] emission lines suggest quasar-driven outflow possibly influencing star formation. Direct stellar velocity dispersion measurements reveal one galaxy follows the local black hole mass-sigma_* relation while the other is overmassive. The existence of massive post-starburst galaxies hosting billion-solar-mass BHs in short-lived quasar phases suggests SMBHs and host galaxies played a major role in each other's rapid early formation.
format Preprint
id arxiv_https___arxiv_org_abs_2409_07113
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle A Post-Starburst Pathway for the Formation of Massive Galaxies and Black Holes at z>6
Onoue, Masafusa
Ding, Xuheng
Silverman, John D.
Matsuoka, Yoshiki
Izumi, Takuma
Strauss, Michael A.
Ward, Charlotte
Phillips, Camryn L.
Ito, Kei
Andika, Irham T.
Aoki, Kentaro
Arita, Junya
Baba, Shunsuke
Bieri, Rebekka
Bosman, Sarah E. I.
Eilers, Anna-Christina
Fujimoto, Seiji
Habouzit, Melanie
Haiman, Zoltan
Imanishi, Masatoshi
Inayoshi, Kohei
Iwasawa, Kazushi
Jahnke, Knud
Kashikawa, Nobunari
Kawaguchi, Toshihiro
Kohno, Kotaro
Lee, Chien-Hsiu
Li, Junyao
Lupi, Alessandro
Lyu, Jianwei
Nagao, Tohru
Overzier, Roderik
Schindler, Jan-Torge
Schramm, Malte
Scoggins, Matthew T.
Shimasaku, Kazuhiro
Toba, Yoshiki
Trakhtenbrot, Benny
Trebitsch, Maxime
Treu, Tommaso
Umehata, Hideki
Venemans, Bram
Vestergaard, Marianne
Volonteri, Marta
Walter, Fabian
Wang, Feige
Yang, Jinyi
Zhang, Haowen
Astrophysics of Galaxies
Cosmology and Nongalactic Astrophysics
Understanding the rapid formation of supermassive black holes (SMBHs) in the early universe requires insight into stellar mass growth in host galaxies. Here, we present NIRSpec rest-frame optical spectra and NIRCam imaging from JWST of two galaxies at z>6, both hosting moderate-luminosity quasars. These galaxies exhibit Balmer absorption lines, similar to low-redshift post-starburst galaxies. Our analyses of the medium-resolution spectra and multiband photometry show bulk of the stellar mass (log (M_* / M_sun) > 10.6) formed in starburst episodes at redshift 9 and 7. One of the galaxies shows a clear Balmer break and lacks spatially resolved H alpha emission. It falls well below the star formation main sequence at z = 6, indicating quiescence. The other is transitioning to quiescence; together, these massive galaxies are among the most distant post-starburst systems known. The blueshifted wings of the quasar [O III] emission lines suggest quasar-driven outflow possibly influencing star formation. Direct stellar velocity dispersion measurements reveal one galaxy follows the local black hole mass-sigma_* relation while the other is overmassive. The existence of massive post-starburst galaxies hosting billion-solar-mass BHs in short-lived quasar phases suggests SMBHs and host galaxies played a major role in each other's rapid early formation.
title A Post-Starburst Pathway for the Formation of Massive Galaxies and Black Holes at z>6
topic Astrophysics of Galaxies
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2409.07113