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Article: The Three Frequencies of the Slowly Pulsating B Star, HD1976.(Brief Article)
- Article from:
- Bulletin of the South Carolina Academy of Science
- Article date:
- January 1, 2001
- Author:
CopyrightCOPYRIGHT 2001 South Carolina Academy of Science. This material is published under license from the publisher through the Gale Group, Farmington Hills, Michigan. All inquiries regarding rights should be directed to the Gale Group. (Hide copyright information)
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In this paper we report on an analysis of the pulsating B star HD1976. This star was found to be a variable with a period of 1.06 days by Waelkens et al. (1998, Astron. & Astrophys., 330, 215) through an analysis of Hipparcos photometry. We put it on the observing program of the Four College Consortium Automatic Photoelectric Telescope (FCAPT) in late 1999. We have confirmed the Hipparcos period, finding a period of 1.06 days (0.939 c/d) in both the Hipparcos and the FCAPT data. We have also tentatively identified a second term with a ...
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... ... described was supported in part by NIH Grant Number RR-6 P20 RR16461-03 from the BRIN Program of the National Center for Research Resources. Jeremy Johnson, Linda Jones Department of Physics and Astronomy College of Charleston, EPSCoR
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