Characterizing the Low-mass Pre-main-sequence Population in the Low-metallicity Star-forming Region Dolidze 25 Using VLT-MUSE

The metallicity of the star-forming environment is a fundamental parameter shaping the evolution of protoplanetary disks and the formation of planetary systems, yet its influence remains poorly constrained. We present a spectroscopic study of low-mass pre-main-sequence (PMS) stars ( M  < 1 M _⊙ ) in...

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Hlavní autoři:	Mizna Ashraf, Jessy Jose, Gregory J. Herczeg, Min Fang, Varsha Ramachandran, Carlo F. Manara, Christian Schneider, Megan Reiter, Kiran Kumar Sunil
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	IOP Publishing 2026-01-01
Edice:	The Astrophysical Journal
Témata:	Pre-main sequence stars Stellar accretion Low mass stars Metallicity
On-line přístup:	https://doi.org/10.3847/1538-4357/ae28cf
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