Volume 390, Number 3, August II 2002
|Page(s)||1023 - 1026|
|Section||Interstellar and circumstellar matter|
|Published online||14 August 2002|
photometry of the CP stars HR 149, HD 32966, HD 171782, and HR 7911*
Department of Physics, The Citadel, 171 Moultrie Street, Charleston, SC 29409, USA
Corresponding author: Saul J. Adelman, firstname.lastname@example.org
Accepted: 23 May 2002
Differential Strömgren observations from the Four College Automated Photoelectric Telescope (FCAPT) are presented for the CP stars HR 149 and HR 7911 and the mCP stars HD 32966 and HD 171782. The Mercury-Manganese star HR 149 is found to be constant while HR 7911 with a period of 5.9617 days probably has a component which is a magnetic CP star. Improved periods were derived for HD 32966 and HD 171782 of 3.0927 and 4.4674 days, respectively. The former is a rather large amplitude mCP star. Both have at least one light curve different in shape from the others observed.
Key words: stars: chemically peculiar / stars: individual: HR 149 / stars: individual: HD 32966 / stars: individual: HD 171782 / stars: individual: HR 7911
© ESO, 2002
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