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HD 5511


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Intermediate band photometry of late-type stars. II - Some stellar groups
Observations on the (R, I) system and a modified Stromgren system ofmembers of six stellar groups are used to demonstrate the chemicalhomogeneity of some 70% or 80% of the members assigned to the groups onthe basis of kinematics. The groups discussed are the Hyades, Wolf 630,Arcturus, Groombridge 1830, and Kapteyn's Star Groups as well as ananonymous group of a half dozen subdwarfs with (U, V) near (-150, -320)km/s. Standards for a previously described photometric system areextended, and additional F- and G-type standards for the (R, I) systemare presented. A simple relation is derived for computing the Fe/Habundance ratio for most stars in the corrected (R-I) interval from +0.2to +0.45 magnitude.

Asteroid spectral reflectivities.
Abstract image available at:http://adsabs.harvard.edu/abs/1973AJ.....78..126C

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观测天体数据

星座:鳳凰座
右阿森松:00h56m14.47s
赤纬:-52°34'47.0"
视星:9.286
右阿森松适当运动:-1.7
赤纬适当运动:8.3
B-T magnitude:9.694
V-T magnitude:9.32

目录:
适当名称   (Edit)
HD 1989HD 5511
TYCHO-2 2000TYC 8473-80-1
USNO-A2.0USNO-A2 0300-00273776
HIPHIP 4388

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