TESS Investigation—Demographics of Young Exoplanets (TI-DYE). II. A Second Giant Planet in the 17 Myr System HIP 67522

The youngest (<50 Myr) planets are vital to understand planet formation and early evolution. The 17 Myr system HIP 67522 is already known to host a giant (≃10 R _⊕ ) planet on a tight orbit. In their discovery paper, Rizzuto et al. reported a tentative single-transit detection of an additional plane...

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Váldodahkkit:	Madyson G. Barber, Pa Chia Thao, Andrew W. Mann, Andrew Vanderburg, Mayuko Mori, John H. Livingston, Akihiko Fukui, Norio Narita, Adam L. Kraus, Benjamin M. Tofflemire, Elisabeth R. Newton, Joshua N. Winn, Jon M. Jenkins, Sara Seager, Karen A. Collins, Joseph D. Twicken
Materiálatiipa:	Artigo
Giella:	Inglês
Almmustuhtton:	IOP Publishing 2024-01-01
Ráidu:	The Astrophysical Journal Letters
Fáttát:	Exoplanets Transit photometry Stellar activity Exoplanet evolution Young stellar objects
Liŋkkat:	https://doi.org/10.3847/2041-8213/ad77d9
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