Abstract
The best way to test planet formation is to find planets in diverse environments. Circumbinary planets have provided that. Once hidden to radial velocities, the BEBOP RV survey has re-discovered Kepler-16b, found a brand new planet BEBOP-1c/TOI-1338c, and has many more data for more treasures. The BEBOP RV program also touches photometric work with TESS and the EBLM survey for low-mass eclipsing binaries. I will discuss the past, present and future of BEBOP, and the implications for planet formation.
Original language | English |
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Article number | 2024n4i614p07 |
Pages (from-to) | 1-2 |
Number of pages | 2 |
Journal | Bulletin of the American Astronomical Society |
Volume | 56 |
Issue number | 4 |
Publication status | Published - 3 Apr 2024 |
Event | AASTCS 10: Extreme Solar Systems V - Te Pae Christchurch Convention Centre, Christchurch, New Zealand Duration: 16 Mar 2024 → 21 Mar 2024 https://aas.org/meetings/exssV |