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Inside-out growth in the early Universe: a core in a vigorously star-forming disc

Authors :
Baker, William M.
Tacchella, Sandro
Johnson, Benjamin D.
Nelson, Erica
Suess, Katherine A.
D'Eugenio, Francesco
Curti, Mirko
de Graaff, Anna
Ji, Zhiyuan
Maiolino, Roberto
Robertson, Brant
Scholtz, Jan
Alberts, Stacey
Arribas, Santiago
Boyett, Kristan
Bunker, Andrew J.
Carniani, Stefano
Charlot, Stephane
Chen, Zuyi
Chevallard, Jacopo
Curtis-Lake, Emma
Danhaive, A. Lola
DeCoursey, Christa
Egami, Eiichi
Eisenstein, Daniel J.
Endsley, Ryan
Hausen, Ryan
Helton, Jakob M.
Kumari, Nimisha
Looser, Tobias J.
Maseda, Michael V.
Puskás, Dávid
Rieke, Marcia
Sandles, Lester
Sun, Fengwu
Übler, Hannah
Williams, Christina C.
Willmer, Christopher N. A.
Witstok, Joris
Baker, William M.
Tacchella, Sandro
Johnson, Benjamin D.
Nelson, Erica
Suess, Katherine A.
D'Eugenio, Francesco
Curti, Mirko
de Graaff, Anna
Ji, Zhiyuan
Maiolino, Roberto
Robertson, Brant
Scholtz, Jan
Alberts, Stacey
Arribas, Santiago
Boyett, Kristan
Bunker, Andrew J.
Carniani, Stefano
Charlot, Stephane
Chen, Zuyi
Chevallard, Jacopo
Curtis-Lake, Emma
Danhaive, A. Lola
DeCoursey, Christa
Egami, Eiichi
Eisenstein, Daniel J.
Endsley, Ryan
Hausen, Ryan
Helton, Jakob M.
Kumari, Nimisha
Looser, Tobias J.
Maseda, Michael V.
Puskás, Dávid
Rieke, Marcia
Sandles, Lester
Sun, Fengwu
Übler, Hannah
Williams, Christina C.
Willmer, Christopher N. A.
Witstok, Joris
Publication Year :
2023

Abstract

The physical processes that establish the morphological evolution and the structural diversity of galaxies are key unknowns in extragalactic astrophysics. Here we report the finding of the morphologically-mature galaxy JADES-GS+53.18343-27.79097, which existed within the first 700 million years of the Universe's history. This star-forming galaxy with a stellar mass of $10^{8.6}$ solar masses consists of three components, a highly-compact core with a half-light radius of 144 pc, a strongly star-forming disc with a radius of 468 pc, and a star-forming clump, which all show distinctive star-formation histories. The central stellar mass density of this galaxy is within a factor of two of the most massive present-day ellipticals, while being globally 1000 times less massive. The radial profile of the specific star-formation rate is strongly rising toward the outskirts. This evidence strongly suggests the first detection of inside-out growth of a galaxy as a proto-bulge and a star-forming disc in the Epoch of Reionization.<br />Comment: 49 pages, 15 figures, submitted to Nature Astronomy

Details

Database :
OAIster
Publication Type :
Electronic Resource
Accession number :
edsoai.on1405314536
Document Type :
Electronic Resource