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...
محفوظ في:
| المؤلفون الرئيسيون: | , , , , , , , , |
|---|---|
| التنسيق: | Artigo |
| اللغة: | Inglês |
| منشور في: |
IOP Publishing
2024-01-01
|
| سلاسل: | The Astrophysical Journal |
| الموضوعات: | |
| الوصول للمادة أونلاين: | https://doi.org/10.3847/1538-4357/ad8c41 |
| الوسوم: |
لا توجد وسوم, كن أول من يضع وسما على هذه التسجيلة!
|