Multiwavelength observations of a giant flare on CN Leonis: III. Temporal evolution of coronal properties
Stellar flares affect all atmospheric layers from the photosphere over chromosphere and transition region up into the corona. Simultaneous observations in different spectral bands allow to obtain a comprehensive picture of the environmental conditions and the physical processes going on during diffe...
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| Main Authors: | , , |
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| Format: | Article (Journal) |
| Language: | English |
| Published: |
27 May 2010
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| In: |
Astronomy and astrophysics
Year: 2010, Volume: 514, Pages: 1-13 |
| ISSN: | 1432-0746 |
| DOI: | 10.1051/0004-6361/201014012 |
| Online Access: | Resolving-System, lizenzpflichtig, Volltext: https://doi.org/10.1051/0004-6361/201014012 Verlag, lizenzpflichtig, Volltext: https://www.aanda.org/articles/aa/abs/2010/06/aa14012-10/aa14012-10.html 
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| Author Notes: | C. Liefke, B. Fuhrmeister, and J.H.M.M. Schmitt |
| Summary: | Stellar flares affect all atmospheric layers from the photosphere over chromosphere and transition region up into the corona. Simultaneous observations in different spectral bands allow to obtain a comprehensive picture of the environmental conditions and the physical processes going on during different phases of the flare. We investigate the properties of the coronal plasma during a giant flare on the active M dwarf CN Leo observed simultaneously with the UVES spectrograph at the VLT and XMM-Newton. |
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| Item Description: | Gesehen am 28.03.2023 |
| Physical Description: | Online Resource |
| ISSN: | 1432-0746 |
| DOI: | 10.1051/0004-6361/201014012 |