4.7 Article

Filling the gap between synchronized and non-synchronized sdBs in short-period sdBV plus dM binaries with TESS: TIC 137608661, a new system with a well-defined rotational splitting

期刊

出版社

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stac160

关键词

asteroseismology; stars: horizontal branch; stars: individual: TIC137608661; stars: oscillations (including pulsations)

资金

  1. Research Foundation - Flanders (FWO), Belgium
  2. Research Council of KU Leuven, Belgium
  3. Fonds National de la Recherche Scientifique (F.R.S.-FNRS), Belgium
  4. Royal Observatory of Belgium
  5. Observatoire de Geneve, Switzerland
  6. NASA Explorer Program
  7. Danish National Research Foundation [DNRF106]
  8. ESA PRODEX [PEA 4000119301]
  9. Stellar Astrophysics Centre (SAC) at Aarhus University
  10. NASA [NAS 5-26555]
  11. INAF project on 'Stellar evolution and asteroseismology in the context of the PLATO space mission'
  12. Grant Agency of the Czech Republic [GACR 1820083S]
  13. Wroclaw Centre for Networking and Supercomputing [265]
  14. National Science Centre [UMO-2017/26/E/ST9/00703, UMO-2017/25/B/ST9/02218]
  15. Thuringer Landessternwarte Tautenburg, Germany

向作者/读者索取更多资源

A new sdBV+dM reflection-effect binary with an orbital period of 7.21 h has been discovered. Multiple g-mode pulsation frequencies were detected in the Fourier transform of the system, along with rotational triplets of equally spaced frequencies. The analysis suggests a rotation period of 4.6 d and indicates a differential rotation with faster rotation at the surface than in the core.
TIC 137608661/TYC 4544-2658-1/FBS 0938+788 is a new sdBV+dM reflection-effect binary discovered by the TESS space mission with an orbital period of 7.21 h. In addition to the orbital frequency and its harmonics, the Fourier transform of TIC 137608661 shows many g-mode pulsation frequencies from the subdwarf B (sdB) star. The amplitude spectrum is particularly simple to interpret as we immediately see several rotational triplets of equally spaced frequencies. The central frequencies of these triplets are equally spaced in period with a mean period spacing of 270.12 s, corresponding to consecutive l = 1 modes. From the mean frequency spacing of 1.25 mu Hz we derive a rotation period of 4.6 d in the deep layers of the sdB star, significantly longer than the orbital period. Among the handful of sdB+dM binaries for which the sdB rotation was measured through asteroseismology, TIC 137608661 is the non-synchronized system with both the shortest orbital period and the shortest core rotation period. Only NY Vir has a shorter orbital period but it is synchronized. From a spectroscopic follow-up of TIC 137608661 we measure the radial velocities of the sdB star, determine its atmospheric parameters, and estimate the rotation rate at the surface of the star. This measurement allows us to exclude synchronized rotation also in the outer layers and suggests a differential rotation, with the surface rotating faster than the core, as found in few other similar systems. Furthermore, an analysis of the spectral energy distribution of TIC 137608661, together with a comparison between sdB pulsation properties and asteroseismic models, gives us further elements to constrain the system.

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