2024/05/24 by Klaus Bernhard, Christopher Lloyd, C. Lloyd · 1 voice
Physics and Astronomy · #Astrophysical Phenomena and Observations #Stellar, planetary, and galactic studies #Astronomy and Astrophysical Research
paper · pdf · doi:10.1051/0004-6361/202450203
Discs in long-period eclipsing binary systems are rare and can lead to extraordinary eclipsing events. ZTF J185259.31+124955.2 was identified as a candidate disc-eclipsing system through a continuing search programme of ZTF variables with a near-IR excess in the WISE data. Examination of the combined ZTF and ATLAS photometry shows seven eclipses since 2017 with depths of 0. m 34 in all bands on a period of 289.57 ± 0.09 d. The eclipse width is ∼40 d but this and the profile evolve over time. Comparison with library spectra shows that the spectral energy distribution from the available photometry is consistent with an early K-type giant, and fitting black-body profiles suggests T eff ∼ 4000 K for the stellar component, with a cool component having T eff < 500 K. The reddening and distance, and hence the luminosity place the star within the giant branch. The most likely scenario is that the system is in a state of rapid evolution following Case B/C mass transfer into an extended disc around an unseen companion.