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HD 32697


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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:05h07m22.21s
Declination:+46°28'41.3"
Apparent magnitude:8.937
Distance:263.852 parsecs
Proper motion RA:4.6
Proper motion Dec:-11.5
B-T magnitude:9.225
V-T magnitude:8.961

Catalogs and designations:
Proper Names   (Edit)
HD 1989HD 32697
TYCHO-2 2000TYC 3345-253-1
USNO-A2.0USNO-A2 1350-05344477
HIPHIP 23827

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