All submissions of the EM system will be redirected to Online Manuscript Submission System. Authors are requested to submit articles directly to Online Manuscript Submission System of respective journal.

Abstract

Microturbulent Velocity in the Atmospheres of G Spectral Classes Star

Author(s): ZA Samedov and MA Jafarov

The microturbulence is investigated in the atmospheres of some G spectral classes stars by the atmosphere model. The microturbulent velocities are determined on the basis of comparison of the values measured from observation and theoretically calculated equivalent widths of lines FeII. It has been found that the microturbulent velocity (𝜉𝑡 ) depends on the surface gravity (g) in the atmospheres of the star: 𝜉𝑡 decreases with increasing g. The microturbulent velocity is less in the stars with intense atmosphere.


Share this       
Welcome Message
Google Scholar citation report
Citations : 260

Journal of Physics & Astronomy received 260 citations as per Google Scholar report

Indexed In

  • Google Scholar
  • Open J Gate
  • China National Knowledge Infrastructure (CNKI)
  • Cosmos IF
  • Directory of Research Journal Indexing (DRJI)
  • MIAR
  • Secret Search Engine Labs
  • Euro Pub
  • clarivate-web-of-science-logo-vector

Read More

Recommended Conferences

4th International Conference on Physics

Paris, France

9th International Conference on Physics

Edinburgh, Scotland

World Congress on Quantum Physics

Berlin, Germany
Flyer
Global Tech Summit