Components of star formation in NGC 253: Non-negative matrix factorization analysis with the ALCHEMI integrated intensity images
Artikel i vetenskaplig tidskrift, 2025
methods: data analysis
galaxies: individual (NGC 253)
galaxies: star formation
galaxies: starburst
ISM: molecules
Författare
Ryo Kishikawa
Tokyo Metropolitan University
Nanase Harada
The Graduate University for Advanced Studies (SOKENDAI)
National Astronomical Observatory of Japan
Toshiki Saito
University of Shizuoka
Laura Colzi
Consejo Superior de Investigaciones Científicas (CSIC)
Mark Gorski
Northwestern University
Christian Henkel
Max-Planck-Gesellschaft
Chinese Academy of Sciences
Jeffrey G. Mangum
National Radio Astronomy Observatory
Sergio Martin
Atacama Large Millimeter-submillimeter Array (ALMA)
European Southern Observatory Santiago
Sebastien Muller
Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium
Yuri Nishimura
University of Tokyo
Victor M. Rivilla
Consejo Superior de Investigaciones Científicas (CSIC)
Kazushi Sakamoto
Academia Sinica
Paul van der Werf
Universiteit Leiden
Serena Viti
Universiteit Leiden
University College London (UCL)
Publication of the Astronomical Society of Japan
0004-6264 (ISSN) 2053051x (eISSN)
Vol. 77 1 1-20Ämneskategorier (SSIF 2011)
Astronomi, astrofysik och kosmologi
Annan fysik
DOI
10.1093/pasj/psae095