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HD 33297


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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:Cocher
Right ascension:05h11m42.14s
Declination:+46°56'32.2"
Apparent magnitude:7.837
Distance:314.465 parsecs
Proper motion RA:-1.8
Proper motion Dec:-1.8
B-T magnitude:7.927
V-T magnitude:7.845

Catalogs and designations:
Proper Names   (Edit)
HD 1989HD 33297
TYCHO-2 2000TYC 3349-131-1
USNO-A2.0USNO-A2 1350-05456363
HIPHIP 24198

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