Modeling Ionized Gas in the Small Magellanic Cloud: The Wolf–Rayet Nebula N76

Modeling Ionized Gas in the Small Magellanic Cloud: The Wolf–Rayet Nebula N76

We present Cloudy modeling of infrared emission lines in the Wolf–Rayet (WR) nebula N76 caused by one of the most luminous and hottest WR stars in the low metallicity Small Magellanic Cloud. We use spatially resolved mid-infrared Spitzer/InfRared Spectrograph and far-infrared Herschel/PACS spectrosc...

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Bibliographic Details
Main Authors: Elizabeth Tarantino, Alberto D. Bolatto, Rémy Indebetouw, Mónica Rubio, Karin M. Sandstrom, J.-D T. Smith, Daniel Stapleton, Mark Wolfire
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Interstellar medium
H II regions
Small Magellanic Cloud
Wolf-Rayet stars
Photoionization
Online Access:https://doi.org/10.3847/1538-4357/ad3def

Internet

https://doi.org/10.3847/1538-4357/ad3def

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