A&A 368, 225-229 (2001)
DOI: 10.1051/0004-6361:20000568
photometry of the CP stars HR 5341, HD 142070, HR 6967,
and HR 8434
Saul J. Adelman Department of Physics, The Citadel, 171 Moultrie Street, Charleston, SC 29409, USA
(Received 20 November 2000 / Accepted 21 December 2000)
Abstract
Differential Strömgren uvby observations from the Four College
Automated Photoelectric Telescope (FCAPT) are presented for the mCP stars
HD 142070, HR 6967, and HR 8434 and the CP star HR 5341. The latter star is
found to be constant. Improved periods were derived for HD 142070, 3.37189 d,
HR 6967, 3.91227 d, and HR 8434, 1.43237 d. Further observations of HD 142070
are needed to phase the magnetic data with the photometry, of HR 6967 to settle
minor discrepancies between y and scaled Geneva V photometry, and of
HR 8434 to resolve small discrepancies between two uvby photometric data
sets.
Key words: stars: chemically peculiar -- stars: individual: HR 5341 -- stars: individual -- HD 142070 -- stars: individual: HR 6967 -- stars: individual: HR 8434
Offprint request: Saul J. Adelman, adelmans@citadel.edu
SIMBAD Objects
Tables at the CDS
© ESO 2001
BibSonomy
CiteUlike
Connotea
Del.icio.us
Digg
Facebook