Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-23T20:41:08.915Z Has data issue: false hasContentIssue false
  • English
  • Français

Panchromatic study of the first galaxies in cosmological simulations

Published online by Cambridge University Press:  10 June 2020

Hidenobu Yajima ,
Shohei Arata Open the ORCID record for Shohei Arata [Opens in a new window] ,
Makito Abe  and
Kentaro Nagamine Open the ORCID record for Kentaro Nagamine [Opens in a new window]
Hidenobu Yajima
Affiliation:
Center for Computational Sciences, University of Tsukuba, 1-1-1 Tennodai, Tsukuba, Ibaraki305-8577, Japan email: yajima@ccs.tsukuba.ac.jp
Shohei Arata
Affiliation:
Department of Earth and Space Science, Graduate School of Science, Osaka University, Toyonaka, Osaka560-0043, Japan
Makito Abe
Affiliation:
Center for Computational Sciences, University of Tsukuba, 1-1-1 Tennodai, Tsukuba, Ibaraki305-8577, Japan email: yajima@ccs.tsukuba.ac.jp
Kentaro Nagamine
Affiliation:
Department of Earth and Space Science, Graduate School of Science, Osaka University, Toyonaka, Osaka560-0043, Japan Department of Physics & Astronomy, University of Nevada, Las Vegas, 4505 S. Maryland Pkwy, Las Vegas, NV89154-4002, USA Kavli IPMU (WPI), The University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba, 277-8583, Japan
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Recent discoveries of high-redshift galaxies have revealed the diversity of their physical properties, from normal star-forming galaxies to starburst galaxies. To understand the properties of these observed galaxies, it is crucial to understand the star formation (SF) history, and the radiation properties associated with the SF activity. Here we present the results of cosmological hydrodynamic simulations with zoom-in initial conditions, and show the formation of the first galaxies and their evolution towards observable galaxies at z = 6. In addition, we show their multi-wavelength radiative properties. We find that star formation occurs intermittently due to supernova (SN) feedback at z > 10, and their radiation properties rapidly change with time. We suggest that the first galaxies are bright at UV wavelengths just after the starburst phase, and become extended Lyman-alpha sources. We also show that massive galaxies cause dusty starburst and become bright at infrared wavelengths.

Keywords

galaxies: formationradiative transfermethods: numerical
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S341: Challenges in Panchromatic Modelling with Next Generation Facilities , November 2019 , pp. 240 - 244
Copyright
© International Astronomical Union 2020

References

Dalla Vecchia, C. & Schaye, J. 2012, MNRAS, 426, 14010.1111/j.1365-2966.2012.21704.xCrossRefGoogle Scholar
Finkelstein, S. L., et al. 2013, Nature, 502, 52410.1038/nature12657CrossRefGoogle Scholar
Hashimoto, T.et al. 2018, Nature, 557, 39210.1038/s41586-018-0117-zCrossRefGoogle Scholar
Ouchi, M.et al. 2018, PASJ, 70, 1310.1093/pasj/psx074CrossRefGoogle Scholar
Schaye, J. & Dalla Vecchia, C. 2008, MNRAS, 383, 121010.1111/j.1365-2966.2007.12639.xCrossRefGoogle Scholar
Springel, V. 2005, MNRAS, 364, 110510.1111/j.1365-2966.2005.09655.xCrossRefGoogle Scholar
Yajima, H., Choi, J. -H., & Nagamine, K. 2011, MNRAS, 412, 41110.1111/j.1365-2966.2010.17920.xCrossRefGoogle Scholar
Yajima, H., Li, Y., Zhu, Q., & Abel, T. 2012, MNRAS, 424, 88410.1111/j.1365-2966.2012.21228.xCrossRefGoogle Scholar
Yajima, H., Nagamine, K., Zhu, Q., Khochfar, S., & Dalla Vecchia, C. 2017, ApJ, 846, 3010.3847/1538-4357/aa82b5CrossRefGoogle Scholar
Watson, D.et al. 2015, Nature, 519, 32710.1038/nature14164CrossRefGoogle Scholar