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HD 33762


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Scanner observations of shell stars Phi Persei and Psi Persei
Spectrophotometric energy distribution data of the shell stars Phi Perand Psi Per are reported in the wavelength range 3200-8000 A. Theeffective temperature of these stars is derived by comparison ofobserved energy distribution with theoretical models. Both the starsshow higher values of derived effective temperature. The continuumenergy distribution in the ultraviolet region has also been discussed.

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Observation and Astrometry data

Constellation:Peintre
Right ascension:05h09m22.34s
Declination:-54°14'28.9"
Apparent magnitude:8.713
Distance:84.317 parsecs
Proper motion RA:43.1
Proper motion Dec:61.3
B-T magnitude:9.351
V-T magnitude:8.766

Catalogs and designations:
Proper Names   (Edit)
HD 1989HD 33762
TYCHO-2 2000TYC 8511-1509-1
USNO-A2.0USNO-A2 0300-01591446
HIPHIP 23986

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