UBVRI photometry of Betelgeuse over 23 years since 1999
Abstract
We report the results of our continuous UBVRI-band photometry of Betelgeuse from 1999 to 2022 using the same photometric system. There are two advantages in our observation: (1) we used a photodiode as a detector to avoid saturation, and (2) our data set includes U-band light curve, which is not widely observed in recent CCD photometries. Using our light curves, we conducted the periodicity analysis, and found about 405- and about 2160-day periods. We also discuss the tentative detection of a long-period variation over 20 years or longer. Finally, we discuss the peculiar variation of the U - B color index during the "Great Dimming" event between late 2019 and early 2020.
- Publication:
-
Open European Journal on Variable Stars
- Pub Date:
- November 2022
- DOI:
- 10.5817/OEJV2022-0233
- arXiv:
- arXiv:2211.04512
- Bibcode:
- 2022OEJV..233....1O
- Keywords:
-
- variable stars;
- Betelgeuse;
- photometry;
- data analysis;
- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- 29 pages, 7 figures, 2 tables. Published in OEJV. Full tables available as table1.dat and table2.dat