DETERMINATION OF MICROTURBULENT VELOCITY IN THE ATMOSPHERE OF THE HD217944 (G8IV) STAR

  • admin admin
  • Z.F. Aliyeva
  • Z.A. Samedov
  • U.R. Rustam

Abstract

In the atmosphere of the HD217944 (G8IV) star, the microturbulent velocity is determined for the odd-even and even-odd transitions. Thus, the microturbulent velocity of iron atoms determined on low levels of odd term lines (ξt = 3.5 km/s) is less than the microturbulent velocity (ξt = 4.2 km/s) determined on low levels of even term lines. This indicates that the microturbulent velocity increases towards the upper layers of atmosphere.

Author Biographies

Z.F. Aliyeva

Baku State University

Z.A. Samedov

Shamakhi Astrophysical Observatory named after Nasreddin Tusi  of ANAS

U.R. Rustam

Shamakhi Astrophysical Observatory named after Nasreddin Tusi  of ANAS

Published
2021-12-29
How to Cite
ADMIN, admin et al. DETERMINATION OF MICROTURBULENT VELOCITY IN THE ATMOSPHERE OF THE HD217944 (G8IV) STAR. Astronomy & Astrophysics (CAUCASUS), [S.l.], v. 5, p. 56-64, dec. 2021. ISSN 2449-2914. Available at: <https://sjunijournals.ge/index.php/AA/article/view/54>. Date accessed: 06 oct. 2022.
Section
Articles