Detection of Diffuse Hot Gas around the Young, Potential Superstar Cluster H72.97–69.39

Detection of Diffuse Hot Gas around the Young, Potential Superstar Cluster H72.97–69.39

We present the first Chandra X-ray observations of H72.97–69.39, a highly embedded, potential superstar cluster in its infancy located in the star-forming complex N79 of the Large Magellanic Cloud. We detect particularly hard, diffuse X-ray emission that is coincident with the young stellar objects...

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Bibliographic Details
Main Authors: Trinity L. Webb, Jennifer A. Rodriguez, Laura A. Lopez, Anna L. Rosen, Lachlan Lancaster, Omnarayani Nayak, Anna F. McLeod, Paarmita Pandey, Grace M. Olivier
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Young star clusters
H II regions
Stellar wind bubbles
Online Access:https://doi.org/10.3847/1538-4357/ad8c41
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