Is sigma Sculptoris Really a Chemically Peculiar Star?

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Title in English Is simga Sculptoris Really a Chemically Peculiar Star?
Authors

JANÍK Jan KRTIČKA Jiří MIKULÁŠEK Zdeněk

Year of publication 2015
Type Article in Proceedings
Conference Physics and Evolution of Magnetic and Related Stars
MU Faculty or unit

Faculty of Science

Citation
Field Astronomy and astrophysics
Keywords sigma Scl; spectroscopy; CP stars
Description We have spectroscopically observed the star sigma Scl during two seasons (2011-2012) with the high dispersion spectrograph FEROS (R = 48 000) attached to the 2.2-m MPG/ESO telescope at La Silla. We did not find any spectral changes in a total of 60 obtained spectra. The chemical composition of sigma Scl is very similar to the solar one. We are also unable to find any periodic photometric variations of the star. Consequently, we cannot classify it as a CP star.
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