Abstract
We report the measurement of a spectroscopic transit of TOI-1726c, one of two planets transiting a G-type star with V = 6.9 in the Ursa Major Moving Group (∼400 Myr). With a precise age constraint from cluster membership, TOI-1726 provides a great opportunity to test various obliquity excitation scenarios that operate on different timescales.
| Original language | English |
|---|---|
| Article number | 193 |
| Journal | Astrophysical Journal |
| Volume | 160 |
| Issue number | 4 |
| Number of pages | 8 |
| ISSN | 0004-637X |
| DOIs | |
| Publication status | Published - 2020 |
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