Characterizing Superflares in HR 1099 Using Temporal and Spectral Analysis of XMM-Newton Observations
In the present paper, we analyze three energetic X-ray flares from the active RS CVn binary HR 1099 using data obtained from XMM-Newton. The flare duration ranges from 2.8 to 4.1 hr, with e -folding rise and decay times in the range of 27–38 minutes and 1.3–2.4 hr, respectively, indicating rapid ris...
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| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2024-01-01
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| Series: | The Astronomical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-3881/ad9601 |
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