Year: 2025
Type: conference-paper
Abstract: In this work, we compare the emission fluxes in the 7.7, 21 .m (JWST) ranges, the CO(2-1) lines (ALMA), and the Hα,Hβ, [OIII] . 5 007 lines (ALMA-MUSE) in the starforming regions of the galaxy NGC 1512. Based on the comparison of the fluxes, we concluded that all the studied fluxes correlate with each other, but to varying degrees.
Authors: E. A. Izmodenova, K. I. Smirnova
Institution: Ural Federal University
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W4412584703
