SPECTRAL RESEARCH OF HOT STARS

Authors

  • A. S. Beisebaeva Kazakh national university, faculty of physics and technology Almaty, Kazakhstan
  • S. A. Khohlov Kazakh national university, faculty of physics and technology Almaty, Kazakhstan
  • A. T. Agishev Kazakh national university, faculty of physics and technology Almaty, Kazakhstan
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Abstract

This work is devoted to investigation of the spectra of hot stars. Plotted dependencies of equivalent widths HeIλ4471, HeIλ4713, MgIIλ4481 lines on the spectral class, which shows the correlation between them. So most accurate indicator of temperature is equivalent width of the HeIλ4713 line.

 Key words: spectrum, equivalent width, hot stars

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How to Cite

Beisebaeva, A. S., Khohlov, S. A., & Agishev, A. T. (2021). SPECTRAL RESEARCH OF HOT STARS. THE JOURNAL OF THE OPEN SYSTEMS EVOLUTION PROBLEMS, 17(1), 44–49. Retrieved from https://peos.kaznu.kz/index.php/peos/article/view/81

Issue

Vol. 17 No. 1 (2015): ЖУРНАЛ ПРОБЛЕМ ЭВОЛЮЦИИ ОТКРЫТЫХ СИСТЕМ

Section

ФИЗИКА