Gas conditions of a star-formation selected sample in the first billion years
Artikel i vetenskaplig tidskrift, 2024
galaxies: ISM
galaxies: high-redshift
galaxies: star formation
Författare
Tom Bakx
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
H. Algera
National Astronomical Observatory of Japan
Hiroshima University
B. Venemans
Universiteit Leiden
Laura Sommovigo
Flatiron Institute
S. Fujimoto
The University of Texas at Austin
S. Carniani
Scuola Normale Superiore di Pisa
Masato Hagimoto
Nagoya University
Takuya Hashimoto
University of Tsukuba
Akio K. Inoue
Waseda University
Dragan Salak
Hokkaido University
S. Serjeant
Open University
L. Vallini
Istituto nazionale di astrofisica (INAF)
S. Eales
Cardiff University
Andrea Ferrara
Scuola Normale Superiore di Pisa
Yoshinobu Fudamoto
Chiba University
Chihiro Imamura
Nagoya University
Shigeki Inoue
Hokkaido University
Kirsten Knudsen
Hokkaido University
Hiroshi Matsuo
National Astronomical Observatory of Japan
The Graduate University for Advanced Studies (SOKENDAI)
Yuma Sugahara
National Astronomical Observatory of Japan
Waseda University
Y. Tamura
Nagoya University
Akio Taniguchi
Nagoya University
Satoshi Yamanaka
National Institute of Technology, Toba College
Monthly Notices of the Royal Astronomical Society
00358711 (ISSN) 13652966 (eISSN)
Vol. 532 2 2270-2288Ämneskategorier
Astronomi, astrofysik och kosmologi
Sannolikhetsteori och statistik
Den kondenserade materiens fysik
DOI
10.1093/mnras/stae1613