PHOTOMETRIC ANALYSIS OF THE VARIABILITY OF LBV STARS AND CANDIDATES IN IC 342
Antoniya Valcheva, Petko Nedialkov, Olga Sholukhova, Nikolay Tikhonov, Milen Minev and Andon Kostov
Publication
BOOK OF ABSTRACTS: XIV Serbian-Bulgarian Astronomical Conference, Page 54, https://doi.org/10.69646/14sbac50a
BOOK OF ABSTRACTS: XIV Serbian-Bulgarian Astronomical Conference, 23 - 27 September, 2024, Vrnjačka Banja, Serbia. Editors: Milan S. Dimitrijević, Evgeni Semkov, Zoran Simić, Goran Damljanović, Momchil Dechev
Published: 17. 11. 2024.
Abstract
Luminous blue variables are a class of massive, unstable stars that exhibit significant photometric variability. Their variability can be linked to their significant mass-loss rates, envelope instabilities and sometimes binarity. These factors can affect the star's brightness and spectrum. LBVs are relatively rare, so studying their variability is challenging. To understand their different types of photometric variability, continuous long-term observations are needed.In this study, we present the analysis of the optical light curves of LBV stars and LBV candidates in the galaxy IC 342. Our observations cover time interval of nearly 4 year and were taken in B and R bands with the 2m telescope at NAO Rozhen, Bulgaria. We supplement our photometry with data from the Pan-STARRS catalog DR1 to expand the light curve coverage and to study both microvariability and long-term variability.