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Physical Sciences and Mathematics Commons

Open Access. Powered by Scholars. Published by Universities.®

Astrophysics and Astronomy

Tennessee State University

1995

HD 181943

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Full-Text Articles in Physical Sciences and Mathematics

Chromospherically Active Stars. Xiv. A Rediscussion Of The Properties And Evolutionary State Of Hd 181943, Francis C. Fekel, Gregory W. Henry, Douglas S. Hall Jun 1995

Chromospherically Active Stars. Xiv. A Rediscussion Of The Properties And Evolutionary State Of Hd 181943, Francis C. Fekel, Gregory W. Henry, Douglas S. Hall

Information Systems and Engineering Management Research Publications

The chromospherically active single star HD 181943 was previously proposed as either a pre-main-sequence star seen pole-on or a post-main-sequence subgiant that evolved from an Ap star similar to 53 Cam. It also was found to be a variable star with a 385 day period. We have used new spectroscopic and photometric observations to reevaluate the properties and evolutionary state of this unusual system. We conclude that HD 181943 is a single K1 V star that has recently arrived on the ZAMS. Its emission line fluxes are nearly identical to those of HD 82558= LQ Hya, while its log lithium …