The helium-weak star 33 Geminorum

Details The helium-weak star 33 Geminorum The helium-weak star 33 Geminorum

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..749g&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, Oct. 1985, p. 749-754) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, Sept.-Oc

Astronomy and Astrophysics

Astronomy

6

Electrophotometry, Peculiar Stars, Stellar Spectrophotometry, Field Strength, Helium, Light Curve, Silicon, Stellar Magnetic Fields

Scientific paper

Photometric observations of 33 Gem = HD 49606 in a system close to UBV have revealed light variations with amplitude ≥0m.05 and period 3d.3546 in all colours. The maximum light coincides in phase with the positive magnetic field extremum. The presence of a magnetic field and photometric variability of large amplitude confirms that 33 Gem is a He-weak star with predominance of silicon anomaly.

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