Open access
Oct 2026
Metal-poor molecular clouds in dwarf galaxies at parsec-scale resolution
Understanding how stars form at low metallicity is challenging because the usual probe of the molecular gas reservoir, carbon monoxide (CO) emission, is faint, and tends to be concentrated in parsec-scale clumps. To overcome this difficulty in our study of molecular clouds in metal-poor environments, we have acquired ̧...
L. Hunt, M. Heyer, U. Lisenfeld et al.
· Astronomy & Astrophysics · 0 citations