Large Population of ALMA Galaxies at z > 6 with Very High [O iii] 88 μm to [C ii] 158 μm Flux Ratios: Evidence of Extremely High Ionization Parameter or PDR Deficit?-Reference-Cited by-同舟云学术

Large Population of ALMA Galaxies at z > 6 with Very High [O iii] 88 μm to [C ii] 158 μm Flux Ratios: Evidence of Extremely High Ionization Parameter or PDR Deficit?

Published:2020-06-17 Issue:2 Volume:896 Page:93
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Harikane Yuichi^ORCID,Ouchi Masami^ORCID,Inoue Akio K.,Matsuoka Yoshiki,Tamura Yoichi^ORCID,Bakx Tom,Fujimoto Seiji^ORCID,Moriwaki Kana,Ono Yoshiaki,Nagao Tohru^ORCID,Tadaki Ken-ichi^ORCID,Kojima Takashi^ORCID,Shibuya Takatoshi,Egami Eiichi,Ferrara Andrea^ORCID,Gallerani Simona,Hashimoto Takuya^ORCID,Kohno Kotaro^ORCID,Matsuda Yuichi^ORCID,Matsuo Hiroshi,Pallottini Andrea,Sugahara Yuma^ORCID,Vallini Livia^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/ab94bd/pdf

Reference142 articles.

1. The H ii Region/PDR Connection: Self‐consistent Calculations of Physical Conditions in Star‐forming Regions

2. The Hyper Suprime-Cam SSP Survey: Overview and survey design

3. ALMA uncovers the [C ii] emission and warm dust continuum in a z = 8.31 Lyman break galaxy

4. The z = 7.54 Quasar ULAS J1342+0928 Is Hosted by a Galaxy Merger

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