Balmer breaks in simulated galaxies at z > 6

Christian Binggeli, Erik Zackrisson, Xiangcheng Ma, Akio K. Inoue, Anton Vikaeus, Takuya Hashimoto, Ken Mawatari, Ikkoh Shimizu, Daniel Ceverino

研究成果: Article査読

4 被引用数 (Scopus)

抄録

Photometric observations of the spectroscopically confirmed z ≈ 9.1 galaxy MACS1149-JD1 have indicated the presence of a prominent Balmer break in its spectral energy distribution, which may be interpreted as due to very large fluctuations in its past star formation activity. In this paper, we investigate to what extent contemporary simulations of high-redshift galaxies produce star formation rate variations sufficiently large to reproduce the observed Balmer break of MACS1149-JD1. We find that several independent galaxy simulations are unable to account for Balmer breaks of the inferred size, suggesting that MACS1149-JD1 either must be a very rare type of object or that our simulations are missing some key ingredient. We present predictions of spectroscopic Balmer break strength distributions for z ≈ 7-9 galaxies that may be tested through observations with the upcoming James Webb Space Telescope and also discuss the impact that various assumptions on dust reddening, Lyman continuum leakage, and deviations from a standard stellar initial mass function would have on the results.

本文言語English
ページ(範囲)3827-3835
ページ数9
ジャーナルMonthly Notices of the Royal Astronomical Society
489
3
DOI
出版ステータスPublished - 2019

ASJC Scopus subject areas

  • 天文学と天体物理学
  • 宇宙惑星科学

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