CHEMICAL COMPOSITION AND EVOLUTIONARY STATUSOF SPECTRAL BINARY STAR 12 PER

Автор(и)

  • V. V. Leushin Special Astrophysical Observatory Nizhnij Arkhyz, Zelenchukskij region, Karachai-Cirkassian Republic 369167 Russia ; Southern Federal University 105 Bolshaya Sadovaya Str., Rostov-on-Don 344006 Russia, Russian Federation
  • M. K. Kuznetsov Southern Federal University 105 Bolshaya Sadovaya Str., Rostov-on-Don 344006 Russia; Institute of Astronomy of the Russian Academy of Sciences Department in Terskol IC AMER Terskol Observatory, Kabardino-Balkaria Republic, 361605 Russia, Russian Federation

DOI:

https://doi.org/10.18524/1810-4215.2008.21.86859

Ключові слова:

stars, binary, spectroscopic and interferometric binary, individual, 12 Per.

Анотація

The star 12 Per is known as a spectroscopic and interferometeric binary. The high resolution spectra in 3700 - 8000 Å band were obtained with the 2 m telescope at Peak Terskol. A detailed analysis of the atmosphere of system's components was carried out using the collected data.

Посилання

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Опубліковано

2008-12-20

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