Звезды солнечного типа с низким уровнем активности, близким к солнечномустатья
Информация о цитировании статьи получена из
Web of Science,
Scopus
Статья опубликована в журнале из списка Web of Science и/или Scopus
Дата последнего поиска статьи во внешних источниках: 20 ноября 2019 г.
Аннотация:Data on the variability of the continuum optical emission are used for the first time to estimate the degree of spotting in stars with activity levels similar to that of the sun. It is shown that the amount of spotting increases gradually from the sun to the highly spotted stars for which Alekseev and Gershberg constructed the zonal model for the distribution of spots. A close relationship is found between spotting and the power of the x-ray emission from stars with widely varying levels of activity.