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HD 13056


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Multivariate statistical analysis of OB stars around H and Chi Persei
A multivariate statistical analysis has been carried out on 49 OB starshaving radial velocities and distance moduli in a field around h and ChiPersei. A hierarchical cluster analysis, combined with discriminantanalysis, has revealed the probable presence of two groups: onebelonging to the Perseus spiral arm (mean distance 2100 pc), the otherlocated at a distance of 1150 pc. Comparison of the difference in meanradial velocities of the groups with the value predicted by the formulaof Oort also supports the result obtained.

Spectral and Luminosity Classifications and Measurements of the Strength of Cyanogen Absorption for Late-Type Stars from Objective-Prism Spectra.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1961ApJ...134..809Y&db_key=AST

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Observation and Astrometry data

Constellation:Bélier
Right ascension:02h08m14.08s
Declination:+23°56'11.9"
Apparent magnitude:7.99
Proper motion RA:103
Proper motion Dec:35.1
B-T magnitude:9.235
V-T magnitude:8.093

Catalogs and designations:
Proper Names   (Edit)
HD 1989HD 13056
TYCHO-2 2000TYC 1758-1860-1
USNO-A2.0USNO-A2 1125-00686685
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