<i>IXPE</i> View of BH XRBs during the First 2.5 Years of the Mission
Accreting stellar-mass black holes represent unique laboratories for studying matter and radiation under the influence of extreme gravity. They are highly variable sources going through different accretion states, showing various components in their X-ray spectra from the thermal emission of the acc...
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| Asıl Yazarlar: | , , , , , , , , , , , , , , |
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| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
MDPI AG
2024-09-01
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| Seri Bilgileri: | Galaxies |
| Konular: | |
| Online Erişim: | https://www.mdpi.com/2075-4434/12/5/54 |
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