The Discovery of a Planetary Companion Interior to Hot Jupiter WASP-132 b

The Discovery of a Planetary Companion Interior to Hot Jupiter WASP-132 b

<jats:title>Abstract</jats:title> <jats:p>Hot Jupiters are generally observed to lack close planetary companions, a trend that has been interpreted as evidence for high-eccentricity migration. We present the discovery and validation of WASP-132 c (TOI-822.02), a 1.8...

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Bibliographic Details
Main Authors: Hord, Benjamin J, Colón, Knicole D, Berger, Travis A, Kostov, Veselin, Silverstein, Michele L, Stassun, Keivan G, Lissauer, Jack J, Collins, Karen A, Schwarz, Richard P, Sefako, Ramotholo, Ziegler, Carl, Briceño, César, Law, Nicholas, Mann, Andrew W, Ricker, George R, Latham, David W, Seager, S, Winn, Joshua N, Jenkins, Jon M, Bouma, Luke G, Falk, Ben, Torres, Guillermo, Twicken, Joseph D, Vanderburg, Andrew
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Format: Article
Language:English
Published: American Astronomical Society 2023
Online Access:https://hdl.handle.net/1721.1/148489

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https://hdl.handle.net/1721.1/148489

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