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HD 216926

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Pulkovo compilation of radial velocities for 35495 stars in a common system. Not Available
Prediction of spectral classification from photometric observations - Application of the UVBY beta photometry and the MK spectra classification. II - General case Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1980A&A....85...93M&db_key=AST
Prediction of spectral classification from photometric observations-application to the UVBY beta photometry and the MK spectral classification. I - Prediction assuming a luminosity class An algorithm based on multiple stepwise and isotonic regressions isdeveloped for the prediction of spectral classification from photometricdata. The prediction assumes a luminosity class with reference touvbybeta photometry and the MK spectral classification. The precisionattained is about 90 percent and 80 percent probability of being withinone spectral subtype respectively for luminosity groups I and V and forluminosity groups III and IV. A list of stars for which discrepanciesappear between photometry and spectral classification is given.
The influence of interstellar absorption on measured strengths of the Balmer discontinuity The definition of the Balmer-discontinuity strength from observationalspectrophotometric data is discussed in relation to detailed results onthe wavenumber dependence of the interstellar absorption. The break inthe interstellar absorption curve at a wavenumber of about 2.33permicrons is found to introduce systematic errors in many currentlydefined strengths of the Balmer discontinuity. The errors should beproportional to the amount of the color excess caused by interstellarabsorption. Using the interstellar absorption curves established byDivan (1954) and by Nandy (1964) theoretical relations are derivedbetween the amount of interstellar absorption and the correspondinginfluence on the Balmer-discontinuity strength. These linear relationsare confirmed through tests on larger sets of observational data. At thesame time the derived relations are useful as correction formulas.
Detection of errors in spectral classification by cluster analysis Cluster analysis methods are applied to the photometric catalogue ofuvby-beta measurements by Hauck and Lindemann (1973) and point out 249stars the spectral type of which should be reconsidered or thephotometric indices of which should be redetermined.
Internal motions in the association Cep OB3. Abstract image available at:http://adsabs.harvard.edu/abs/1973AJ.....78..185G
Spectral classification in the association III Cephei and the ratio of total-to-selective absorption. Abstract image available at:http://adsabs.harvard.edu/abs/1970AJ.....75.1001G
Photoelectric measures of the 4430 A diffuse interstellar band Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1963MNRAS.125..141W&db_key=AST
Photoelectric Photometry of the Association III Cephei. Abstract image available at:http://adsabs.harvard.edu/abs/1959ApJ...130...69B

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Observation and Astrometry data

Constellation:	Céphée
Right ascension:	22^h55^m52.62^s
Declination:	+63Â°28'23.1"
Apparent magnitude:	8.904
Distance:	515.464 parsecs
Proper motion RA:	-0.3
Proper motion Dec:	-5.6
B-T magnitude:	9.165
V-T magnitude:	8.926

Catalogs and designations:

Proper Names
HD 1989	HD 216926
TYCHO-2 2000	TYC 4282-508-1
USNO-A2.0	USNO-A2 1500-09393193
HIP	HIP 113236

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