My talk at Towards Other Earths III, in Porto Portugal, on Monday July 17, at 5:10 PM.
The talk is about our recently submitted paper here:
https://arxiv.org/abs/2307.08959
Note that the HAT-P-67 stellar and planet properties reported on slides 20 and 21 reflect the previously published values from Zhou et al. 2017. Our new paper (link above) slightly refines these values from revised Gaia DR3 distance, use of new isochrones, and more numerous RV samples with HPF (albeit still consistent with an RV non-detection). See the paper for more information.
Slide 38 shows an animation from Thorngren, Lee, & Lopez 2023 available on the HTML version of the ApJ website:
https://iopscience.iop.org/article/10.3847/2041-8213/acbd35
The top-down orbit on slides 28 - 31 is merely a cartoon to emphasize the leading nature ot the tail, and not its actual orbital location-- a genuine planetary wind consistent with the outflow will initially reside at orbital separations closer into the star, and not directly on top of the planet orbit.