Period analysis of a Blazhko star V0346 Draconis

Warning

This publication doesn't include Faculty of Education. It includes Faculty of Science. Official publication website can be found on muni.cz.
Authors

LIŠKA Jiří SKARKA Marek

Year of publication 2015
Type Article in Periodical
Magazine / Source Open European Journal on Variable Stars
MU Faculty or unit

Faculty of Science

Citation
Web http://var.astro.cz/oejv/oejv.php?oejv=173
Field Astronomy and astrophysics
Keywords photometry;RR Lyrae;CCD;Blazhko effect;variable star
Description Period analysis of an RRab star V0346 Dra based on photometric measurements from NSVS and DASCH projects is presented. We confirm light curve modulation known from literature and estimate modulation period for the first time. NSVS measurements spanning one year allowed us to determine the length of the Blazhko cycle as 101(2) d. This value is close to 103.65(2)-day period estimated from photographic measurements from the DASCH project which have a lower quality but 92-year long timebase. Blazhko effect causes well apparent phase and amplitude modulation easily visible in O-C diagram and in maximum-O-C dependency.
Related projects:

You are running an old browser version. We recommend updating your browser to its latest version.