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The nitrogen abundance in the atmospheres of single and binary stars
The nitrogen abundances for 47 single, 11 visual double, and 41 closebinary stars are obtained from high-dispersion Wlambdadeterminations of nitrogen lines using atmospheric models andtheoretical calculations of N II lines, taking LTE errors into account.The mean value of lg N(N) is found to be 8.05 for single stars, 8.50 forclose binaries, and 8.15 for visual double stars. A correlation is foundbetween the nitrogen abundance and the helium and carbon abundances. Itis suggested that considerable mixing between the central part of starsand the atmosphere occurs in binary stars.
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Gözlemler ve gökölçümü verileri
| Takýmyýldýz: | Boga |
| Sað Açýklýk: | 03h56m37.44s |
| Yükselim: | +23°35'44.0" |
| Görünürdeki Parlaklýk: | 8.372 |
| özdevim Sað Açýklýk: | -2.2 |
| özdevim Yükselim: | -6.3 |
| B-T magnitude: | 10.169 |
| V-T magnitude: | 8.521 |
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