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HD 34806


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The determination of the zero point of the wavelength scale on stellar spectrograms
A novel method for determining the zero point of the wavelength scale(lambda0) on low-spectral-resolution spectrograms obtainedwith an objective plasma is presented. The method was applied to a groupof 100 stars belonging to the B-G spectral classes. Near-UV spectrogramsof these stars were obtained by the Orion-2 space observatory.Equivalent widths were obtained for the resonance doublet of Mg II 2800A in the spectra of the stars studied.

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Observation and Astrometry data

Constellation:Auriga
Right ascension:05h22m24.30s
Declination:+45°49'54.9"
Apparent magnitude:9.166
Proper motion RA:5.6
Proper motion Dec:-4.4
B-T magnitude:9.318
V-T magnitude:9.179

Catalogs and designations:
Proper Names
HD 1989HD 34806
TYCHO-2 2000TYC 3358-3030-1
USNO-A2.0USNO-A2 1350-05703252
HIPHIP 25099

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