Energizing star formation: the cosmic-ray ionization rate in NGC 253 derived from ALCHEMI measurements of H3O+ and SO

Author(s):
Holdship, J.R.; Mangum, J.G.; Viti, S. (0000-0001-8504-8844); Behrens, E.; Harada, N.; Martín, S.; Sakamoto, K.; Muller, S.; Tanaka, K.; Nakanishi, K.; Herrero-Illana, R.; Yoshimura, Y.; Aladro, R.; Colzi, L.; Emig, K.L.; Henkel, C.; Nishimura, Y.; Rivilla, V.M.; Werf, P.P. van der (0000-0002-4389-832x)
Published
2022
Publication type
Article / Letter to editor
Starburst GalaxiesInterstellar MediumActive GalaxiesInterstellar Abundances157084717832Astrophysics - Astrophysics of Galaxies
Date issued
2022
Language
English
Is part of
The Astrophysical Journal (2022), No. 2, 89
hdl
1887/3561648
doi
10.3847/1538-4357/ac6753
URL
https://ui.adsabs.harvard.edu/abs/2022ApJ...931...89H