SDSS-V LVM: Resolving physical conditions in the Trifid Nebula
Aims. The chemical abundance of the interstellar medium sets the initial conditions for star formation and provides a probe of chemical galaxy evolution models. However, unresolved inhomogeneities in the electron temperature can lead to a systematic underestimation of the abundances. We aim to directly test this effect. Methods. We used the SDSS-V
Sattler, Natascha et al.
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2026