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Cyanogen strengths, mixing and supermetallicity in G and K giants
Wide visual binaries consisting of a G or K giant in physicalassociation with an F dwarf, observed using DDO and ubvy photometry,were used to study the possibility of mixing in the giants prior to orduring helium core burning. The two abundance indices, delta m1 of theuvby system, and delta CN of the DDO system, are compared to study thepossibility that mixing from a hydrogen burning region has affected theCN strengths of the giants.
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Observation and Astrometry data
| Constellation: | Poissons |
| Right ascension: | 01h17m28.27s |
| Declination: | +21°05'06.7" |
| Apparent magnitude: | 8.766 |
| Proper motion RA: | -23.1 |
| Proper motion Dec: | -34.1 |
| B-T magnitude: | 9.419 |
| V-T magnitude: | 8.82 |
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