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Additional late-type stars with technetium The results of a survey of 279 late-type giants and supergiants for thespectral lines of the radioactive element technetium (Tc I) at 4297,4262, and 4238 A are presented. The following conclusions are reached:(1) the presence of Tc correlates very strongly with the existence oflight variability; (2) evolutionary MS stars show Tc and spectroscopicMS stars do not show Tc; (3) single S stars show Tc; (4) SC stars showTc; (5) about 75 percent of the C stars show Tc; and (6) Ba II stars donot show Tc. The findings are compatible with predictions from stellarevolution theory.
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Observation and Astrometry data
Constellation: | Orion |
Right ascension: | 06h25m21.52s |
Declination: | +10°48'32.3" |
Apparent magnitude: | 7.403 |
Proper motion RA: | -0.9 |
Proper motion Dec: | -0.4 |
B-T magnitude: | 7.309 |
V-T magnitude: | 7.396 |
Catalogs and designations:
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