Astron. Astrophys. Suppl. Ser.
Volume 123, Number 3, June II 1997
|Page(s)||445 - 447|
|Published online||15 June 1997|
On the possible variability of metallic-line and Mercury-Manganese stars*
Department of Physics, The Citadel, 171 Moultrie Street, Charleston, SC 29409, U.S.A.
Send offprint request to: S.J. Adelman
Accepted: 9 October 1996
Differential Strömgren uvby photometric observations from the 0.75-m Four College Automated Photoelectric Telescope were obtained for three metallic-line and three Mercury-Manganese stars. None were found to be variable. These sharp-lined stars may not be the best tests for class variability as their polar axes are pointed towards the earth. Each presents essentially the same visible hemisphere as it rotates.
Key words: stars: chemically peculiar
Tables 2-7 are available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (184.108.40.206) or via http://cdsweb.u-strasbg.fr/Abstract.html
© European Southern Observatory (ESO), 1997