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Mixing in close binaries
Consideration is given to mixing of matter in radiative zones ofmain-sequence stars which enter close synchronized binary systems. Themixing is created by slow circulation currents which maintain thethermal balance and may be responsible for the excesses of N-14 and H-4and the deficit of C-12 observed in the surface layers of close binarycomponents.
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Observation and Astrometry data
| Constellation: | Ιχθείς |
| Right ascension: | 00h26m54.28s |
| Declination: | +08°33'46.0" |
| Apparent magnitude: | 8.59 |
| Proper motion RA: | 4.4 |
| Proper motion Dec: | 4.2 |
| B-T magnitude: | 10.107 |
| V-T magnitude: | 8.716 |
Catalogs and designations:
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