LINES SELECTION TO DETERMINE THE CHEMICAL COMPOSITION OF STARS IN THE RANGE -3 <= [FE/H] <= -0.7
Using the spectra obtained with echelle spectrograph SOPHIE (1.93 m telescope, OHP, France) and the data from about 20 papers of various authors, we have compiled a list for around four thousand lines of different chemical elements. Based on the spectra of the Sun and stars and also synthetic spectr...
Main Authors: | N. Yu. Basak, T. V. Mishenina |
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Format: | Article |
Language: | English |
Published: |
Odessa I. I. Mechnykov National University
2012-11-01
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Series: | Odessa Astronomical Publications |
Online Access: | http://oap.onu.edu.ua/article/view/83344 |
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