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HD 34380


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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.

Photoelectric Observations of the Eclipsing Binary IM Aurigae
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Observation and Astrometry data

Constellation:Auriga
Right ascension:05h19m10.69s
Declination:+45°00'41.4"
Apparent magnitude:8.321
Distance:167.785 parsecs
Proper motion RA:1.8
Proper motion Dec:-1.1
B-T magnitude:8.62
V-T magnitude:8.346

Catalogs and designations:
Proper Names   (Edit)
HD 1989HD 34380
TYCHO-2 2000TYC 3358-3093-1
USNO-A2.0USNO-A2 1350-05631073
HIPHIP 24816
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