Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007smma.conf..350s&link_type=abstract
Spectroscopic methods in modern astrophysics. Proceedings of the conference held 13-15 September 2006, Moscow, Russia. Eds. L. M
Astronomy and Astrophysics
Astrophysics
Scientific paper
We report the results of the investigations of chemical composition of close binaries which had gone through the stage of common envelope and which are the remnants of planetary nebular cores. High resolution spectra for different phases of orbital period of V471 Tau were taken by RTT-150 telescope and were investigated by the modified SYNTH program. The spectra show noticeable variability with an appearance of emission components dependent of the orbital period phase. For chemical composition determination, the "solar" oscillator strengths of 700 lines were determined. It was found that the chemical content of V471 Tau is a composite one and is characterized by excess of α-process elements in the contrast to small underabundance of iron-peak elements. An estimation of different element abundances in the star allows to determine their contents in planetary nebular phase.
Bikmaev I. F.
Sakhibullin N. A.
Shigapov R. R.
Shimanskaya N. N.
Shimansky V. V.
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