TOI-1259Ab - a gas giant planet with 2.7 per cent deep transits and a bound white dwarf companion
Abstract
We present TOI-1259Ab, a 1.0RJup gas giant planet transiting a 0.71R⊙ K-dwarf on a 3.48 d orbit. The system also contains a bound white dwarf companion TOI-1259B with a projected distance of ~1600 au from the planet host. Transits are observed in nine TESS sectors and are 2.7 per cent deep - among the deepest known - making TOI-1259Ab a promising target for atmospheric characterization. Our follow-up radial velocity measurements indicate a variability of semiamplitude $K=71\, \rm m\, s^{-1}$, implying a planet mass of 0.44MJup. By fitting the spectral energy distribution of the white dwarf, we derive a total age of $4.08^{+1.21}_{-0.53}$ Gyr for the system. The K dwarf's light curve reveals rotational variability with a period of 28 d, which implies a gyrochronology age broadly consistent with the white dwarf's total age.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- November 2021
- DOI:
- 10.1093/mnras/stab2129
- arXiv:
- arXiv:2101.02707
- Bibcode:
- 2021MNRAS.507.4132M
- Keywords:
-
- planets and satellites: formation;
- binaries: eclipsing;
- stars: individual (TOI-1259);
- stars: low-mass;
- stars: rotation;
- Astrophysics - Earth and Planetary Astrophysics;
- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- Accepted to MNRAS. Some structural changes from first arXiv version but no significant changes to results. One figure got a bit prettier