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HD 104955


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Red horizontal-branch stars in the galactic disk
A quantitative, three-dimensional spectral classification systemdeveloped by Rose (1984), which uses 2.5-A resolution spectra in theblue, has been used to identify a class of red horizontal branch (RHB)stars in the Galactic disk that are similar to those in the 'metal rich'globular cluster M 71. The RHB are denoted as evolved stars by their SrII 4077 line, and are distinguished from post-main sequence starsevolving through the same region of the HR diagram on the basis of theunique appearance of their CN 3883 and 4216 A bands. The RHB starsconsitute at least 5 percent of the entire giant branch population ofthe disk.

UBVRI photometry of north galactic pole K giants
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1970AJ.....75..971H&db_key=AST

The space distribution of late type stars in a North galactic pole region.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1962AJ.....67...37U&db_key=AST

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Observation and Astrometry data

Constellation:Ursa Major
Right ascension:12h05m06.62s
Declination:+47°24'09.1"
Apparent magnitude:8.711
Distance:173.913 parsecs
Proper motion RA:-136.9
Proper motion Dec:39.6
B-T magnitude:9.737
V-T magnitude:8.796

Catalogs and designations:
Proper Names
HD 1989HD 104955
TYCHO-2 2000TYC 3455-364-1
USNO-A2.0USNO-A2 1350-08055169
HIPHIP 58938

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