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HD 1818


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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:Toucan
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:
Proper Names   (Edit)
HD 1989HD 1818
TYCHO-2 2000TYC 8840-1849-1
USNO-A2.0USNO-A2 0225-00099288
HIPHIP 1751

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