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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 direc...

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Principais autores: Sattler Natascha, Méndez-Delgado J. Eduardo, Kreckel Kathryn, Morisset Christophe, Egorov Oleg, Egorova Evgeniya, Nemer Ahmad, Liang Fu-Heng, Sander A. A. C., Roman-Lopes Alexandre, Román-Zúñiga Carlos G., Johnston Evelyn J., Sánchez Sebastián F., Fernández-Trincado José G., Drory Niv, Singh Amrita, Bizyaev Dmitry, Sarbadhicary Sumit K., García Pablo, Mejía-Narváez Alfredo, Blanc Guillermo A.
Formato: Artigo
Idioma:Inglês
Publicado em: EDP Sciences 2026-02-01
coleção:Astronomy & Astrophysics
Assuntos:
ism: abundances
ism: general
hii regions
ism: structure
local insterstellar matter
ism: individual objects: m 20
Acesso em linha:https://www.aanda.org/articles/aa/full_html/2026/02/aa58091-25/aa58091-25.html
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