Components of star formation in NGC 253: Non-negative matrix factorization analysis with the ALCHEMI integrated intensity images
Journal article, 2025
methods: data analysis
galaxies: individual (NGC 253)
galaxies: star formation
galaxies: starburst
ISM: molecules
Author
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
Spanish National Research Council (CSIC)
Mark Gorski
Northwestern University
Christian Henkel
Max Planck Society
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, Space, Earth and Environment, Onsala Space Observatory
Yuri Nishimura
University of Tokyo
Victor M. Rivilla
Spanish National Research Council (CSIC)
Kazushi Sakamoto
Academia Sinica
Paul van der Werf
Leiden University
Serena Viti
Leiden University
University College London (UCL)
Publication of the Astronomical Society of Japan
0004-6264 (ISSN) 2053051x (eISSN)
Vol. 77 1 1-20Subject Categories (SSIF 2011)
Astronomy, Astrophysics and Cosmology
Other Physics Topics
DOI
10.1093/pasj/psae095