THE CHEMICAL COMPOSITION OF THE ACTIVE STARS

Автор(и)

  • L. V. Glazunova Department of Astronomy, Odessa National University; Odessa National Academy of Telecommunications, Ukraine

DOI:

https://doi.org/10.18524/1810-4215.2016.29.84982

Ключові слова:

Stars, binaries, abundances, stars, individual, LX Per, OU Gem, BY Dra, RS CVn

Анотація

The comparison of the results of the studies of the active stars’ chemical composition obtained by different authors has been performed. It was concluded that the difference between the abundances of some elements in active and inactive stars becomes significant (> 3σ) only for the active stars with high chromospheric activity (lgR’HK > -4). This is the case primarily for the light elements, namely Li, Na and Al, as well as heavy elements with Z > 30.

 

Посилання

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Опубліковано

2016-12-01

Номер

Розділ

Астрофізика (зоряні атмосфери, взаємодіючі подвійні системи, змінні зорі)