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Accretion onto the Embedded Protostar L1527 IRS: Insights from JWST NIRSpec and MIRI Observations

Accretion is the primary driver of protostellar evolution, regulating mass assembly and shaping the physical and chemical environments of young stellar objects. Quantifying accretion in the Class 0 protostellar phase is particularly important, yet remains observationally challenging due to high exti...

Ausführliche Beschreibung

Gespeichert in:
Hauptverfasser: W. Blake Drechsler, John J. Tobin, Patrick D. Sheehan, Leslie W. Looney, S. Thomas Megeath, Ewine F. Van Dishoeck, Valentin J. M. Le Gouellec, Thomas P. Greene, Logan Francis, R. Devaraj, Martijn van Gelder, Lee Hartmann, Lukasz Tychoniec, Nuria Calvet, William J. Fischer
Format: Artigo
Sprache:Inglês
Veröffentlicht: IOP Publishing 2026-01-01
Schriftenreihe:The Astrophysical Journal
Schlagworte:
Star formation
Protostars
Stellar accretion disks
Stellar accretion
Online-Zugang:https://doi.org/10.3847/1538-4357/ae4a25
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