Coronal models of late-type stars observed with EXOSAT |
| |
| Institution: | 1. Osservatorio Astrofisico di Arcetri, Firenze, Firenze, Italy;7. Università degli Studi di Firenze, Firenze, Italy;1. University of Sofia, Faculty of Physics, Department of Atomic Physics, 5 James Bourchier Blvd., 1164, Sofia, Bulgaria;2. Institute of Catalysis, Bulgarian Academy of Sciences, Acad. G. Bonchev St., Bldg. 11, 1113, Sofia, Bulgaria |
| |
| Abstract: | Differential emission measure distributions for transition region and corona able to reproduce X-ray and UV emission are investigated. The EXOSAT, EINSTEIN and IUE data for the solar type star K Cet are analyzed. A multitemperature differential emission measure distribution gives a satisfactory fit of the data. |
| |
| Keywords: | |
| 本文献已被 ScienceDirect 等数据库收录！ |
|
