Title | Fig. 2. The brightness behavior of V647 Her based on observations in 2019 and 2022. (a) results of observations in 2022, (b) series of ΔV-magnitudes after primary processing of data in 2019 and 2022, ΔV are determined relative to the comparison star TYC 2082-2143-1, the dotted line marks the maximum brightness level. |
Submission | Distribution of cool starspots on the surface of the red dwarf V647 Her |
Type | author.submit.suppFile.figureResearchMaterials |
Date | 2024-11-26 |
Language | ru |
Supplementary File
File Name | 647609-5015187-1-SP.jpg |
Original file name | Рис_2.jpg |
File Size | 71KB |
Date uploaded | 28.01.2025 22:00 |