First JWST/NIRSpec Spectroscopy of O Stars in the Small Magellanic Cloud

First JWST/NIRSpec Spectroscopy of O Stars in the Small Magellanic Cloud

Determining how much mass is removed by stellar winds is crucial to understanding massive star evolution and feedback. However, traditional spectroscopic diagnostics in the UV and optical are not sensitive enough to characterize weak stellar winds of OB stars in low-metallicity environments. A new t...

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Bibliographic Details
Main Authors: Armin Mang Román, Peter Zeidler, Wolf-Rainer Hamann, Lidia M. Oskinova, M. J. Rickard, S. Reyero Serantes, H. Todt, J. S. Gallagher III, D. Massa, D. Pauli, V. Ramachandran, E. Sabbi, A. A. C. Sander
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Letters
Subjects:
O stars
Small Magellanic Cloud
Stellar winds
Young massive clusters
Stellar luminosities
Stellar atmospheres
Online Access:https://doi.org/10.3847/2041-8213/adcc22
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https://doi.org/10.3847/2041-8213/adcc22

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