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HD 245287


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U, V, W velocity components for the old disk using radial velocities of 1295 stars in the three cardinal Galactic directions
New radial velocities are presented for 1295 stars chosen at random nearthe three cardinal Galactic directions of l = 180 deg, b = 0; l = 90deg, b = 0 deg; and b = 90 deg, giving the distribution in U, V, and W,respectively, from the radial velocities alone. The measurements weremade with the coude spectrograph of the Mount Wilson 100 in. Hookerreflector. The purpose of the program is to set limits on the densitynormalization in the solar neighborhood of the old thin disk, the oldthick disk, and the halo. Many more high-velocity stars are present inthe unbiased sample than expected from previous estimates of thenormalization. The data suggest the density ratios in the solarneighborhood to be about 90 percent, 10 percent, and about 0.5 percentfor the thin disk, thick disk, and halo populations, respectively.

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Observation and Astrometry data

Constellation:Auriga
Right ascension:05h36m34.62s
Declination:+29°01'09.4"
Apparent magnitude:9.462
Proper motion RA:13.5
Proper motion Dec:-27.4
B-T magnitude:9.993
V-T magnitude:9.506

Catalogs and designations:
Proper Names   (Edit)
HD 1989HD 245287
TYCHO-2 2000TYC 1873-722-1
USNO-A2.0USNO-A2 1125-02607292
HIPHIP 26342

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