Supplementary File

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
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Date uploaded 28.01.2025 22:00