arXiv Analytics

Sign in

arXiv:2502.09444 [astro-ph.SR]AbstractReferencesReviewsResources

The orbital parameters of the binary BLAP HD133729 : advantages of the frequency modulation method

Hiromoto Shibahashi, Donald W. Kurtz, Simon J. Murphy

Published 2025-02-13Version 1

We derive all the orbital parameters of the blue large-amplitude pulsator (BLAP) in the binary system HD133729 by exploiting the frequency modulation (FM) method, which is based on the analytical relations between the orbital parameters and a multiplet separated by the orbital frequency in the frequency spectrum of the light curve. Because the FM method uses the entire data through the Fourier transform, it is the most effective use of high-precision photometry data, taken over a long timespan by the TESS space mission, for determining orbital parameters.

Related articles: Most relevant | Search more
arXiv:1801.09926 [astro-ph.SR] (Published 2018-01-30)
SY Mus - search for physical parameters
arXiv:2307.08472 [astro-ph.SR] (Published 2023-07-17)
Markov Chain Monte Carlo applied to the Double Stars of Miller and Pitman
arXiv:0907.3613 [astro-ph.SR] (Published 2009-07-21)
EXOFIT: Bayesian Estimation of Orbital Parameters of Extrasolar Planets