EMPRESS. IV. Extremely metal-poor galaxies including very low-mass primordial systems with M* = 10^4-10^5 M and 2%-3% (O/H): high (Fe/O) suggestive of metal enrichment by hypernovae/pair-instability supernovae

Author(s):
Isobe, Y.; Ouchi, M.; Suzuki, A.; Moriya, T.J.; Nakajima, K.; Nomoto, K.; Rauch, M.; Harikane, Y.; Kojima, T.; Ono, Y.; Fujimoto, S.; Inoue, A.K.; Kim, J.H.; Komiyama, Y.; Kusakabe, H.; Lee, C.-H.; Maseda, M.; Matthee, J.; Michel-Dansac, L.; Nagao, T.; Nanayakkara, T.; Nishigaki, M.; Onodera, M.; Sugahara, Y.; Xu, Y.
Published
2022
Publication type
Article / Letter to editor
5956221569580416Astrophysics - Astrophysics of Galaxies
Date issued
2022
Language
English
Is part of
The Astrophysical Journal (2022), No. 2, 111
hdl
1887/3561808
doi
10.3847/1538-4357/ac3509
URL
https://ui.adsabs.harvard.edu/abs/2022ApJ...925..111I