
Stability of Nonradial Pulsations in the Be Star [MA93]1506
Author(s) -
P. C. Schmidtke,
A. P. Cowley,
A. Udalski
Publication year - 2021
Publication title -
research notes of the aas
Language(s) - English
Resource type - Journals
ISSN - 2515-5172
DOI - 10.3847/2515-5172/ac391c
Subject(s) - photometry (optics) , astrophysics , star (game theory) , radial velocity , stars , physics , astronomy , environmental science
Period analysis of the 1993–2020 MACHO and OGLE photometry for Be star [MA93]1506 reveals non-radial pulsations are present in all observing seasons, with a mean period of 1.09942 ± 0.00018 days.