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Kinematic properties of supergiants in the Perseus spiral arm
Analysis of the space motions of supergiants in the Perseus arm regionindicates that the stellar peculiar-velocity field has a large-scalenonuniformity probably resulting both from the presence of sizablegroups of young stars and from systematic motions in the arm aspredicted by density-wave theory. Proper motions are tabulated for 78stars.
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Observation and Astrometry data
| Constellation: | Tucana |
| Right ascension: | 00h22m10.00s |
| Declination: | -61°17'50.7" |
| Apparent magnitude: | 7.839 |
| Distance: | 318.471 parsecs |
| Proper motion RA: | 34.6 |
| Proper motion Dec: | 13 |
| B-T magnitude: | 9.354 |
| V-T magnitude: | 7.965 |
Catalogs and designations:
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