CAOSP abstracts, Volume: 33, No.: 1, year: 2003
- Author(s): Mikulášek, Z.; Žižňovský, J.; Zverko, J.; Polosukhina, N.S.
- Journal: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 33, no. 1, p. 29-37.
- Date: 02/2003
- Title: Improved period of a slowly rotating cool magnetic CP star HD 188041
- Keyword(s): CP stars, photometry, variability, period
- Pages: 29 -- 37
The ephemeris of variations of the cool magnetic CP star HD 188041
was newly determined using all photometric, magnetic and spectroscopic
observations available. The improved period
P=(223.826±0.040) d is common for all types of variation
observed, all previously mentioned periods were definitely eliminated. The
origin of phase counting
M0=(2 444 981.8±0.6) was put in the
centre of the v light minimum. The effective magnetic field maximum
lies at phase 0.002±0.019. The slightly asymmetric curve of
Gd II line strength has its maximum at -0.031±0.012.
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