HAT-P-39b-HAT-P-41b: Three Highly Inflated Transiting Hot Jupiters

Author(s): Hartman, Joel D.; Bakos, Gaspar Aron; Béky, B; Torres, G; Latham, David W.; et al

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Abstract:	We report the discovery of three new transiting extrasolar planets orbiting moderately bright ( V = 11 . 1, 11 . 7, and 12 . 4) F stars. The planets HAT-P-39b through HAT-P-41b have periods of P = 3 . 5439 days, 4 . 4572 days, and 2 . 6940 days, masses of 0 . 60 M J ,0 . 62 M J , and 0 . 80 M J , and radii of 1 . 57 R J ,1 . 73 R J , and 1 . 68 R J , respectively. They orbit stars with masses of 1 . 40 M ,1 . 51 M , and 1 . 51 M , respectively. The three planets are members of an emerging population of highly inflated Jupiters with 0 . 4 M J <M< 1 . 5 M J and R> 1 . 5 R J.
Publication Date:	Nov-2012
Electronic Publication Date:	9-Oct-2012
Citation:	Hartman, JD, Bakos, GÁ, Béky, B, Torres, G, Latham, DW, Csubry, Z, Penev, K, Shporer, A, Fulton, BJ, Buchhave, LA, Johnson, JA, Howard, AW, Marcy, GW, Fischer, DA, Kovács, G, Noyes, RW, Esquerdo, GA, Everett, M, Szklenár, T, Quinn, SN, Bieryla, A, Knox, RP, Hinz, P, Sasselov, DD, Fúrész, G, Stefanik, RP, Lázár, J, Papp, I, Sári, P. (2012). HAT-P-39b-HAT-P-41b: Three Highly Inflated Transiting Hot Jupiters. \aj, 144 (139 - 139. doi:10.1088/0004-6256/144/5/139
DOI:	doi:10.1088/0004-6256/144/5/139
Type of Material:	Journal Article
Journal/Proceeding Title:	Astronomical Journal
Version:	Final published version. This is an open access article.