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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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dc.contributor.authorHartman, Joel D.-
dc.contributor.authorBakos, Gaspar Aron-
dc.contributor.authorBéky, B-
dc.contributor.authorTorres, G-
dc.contributor.authorLatham, David W.-
dc.contributor.authorCsubry, Zoltan-
dc.contributor.authorPenev, K-
dc.contributor.authorShporer, A-
dc.contributor.authorFulton, BJ-
dc.contributor.authorBuchhave, Lars A.-
dc.contributor.authorJohnson, JA-
dc.contributor.authorHoward, AW-
dc.contributor.authorMarcy, GW-
dc.contributor.authorFischer, DA-
dc.contributor.authorKovács, G-
dc.contributor.authorNoyes, Robert W.-
dc.contributor.authorEsquerdo, GA-
dc.contributor.authorEverett, M-
dc.contributor.authorSzklenár, T.-
dc.contributor.authorQuinn, SN-
dc.contributor.authorBieryla, A-
dc.contributor.authorKnox, RP-
dc.contributor.authorHinz, P-
dc.contributor.authorSasselov, DD-
dc.contributor.authorFúrész, G-
dc.contributor.authorStefanik, RP-
dc.contributor.authorLázár, J.-
dc.contributor.authorPapp, I-
dc.contributor.authorSári, P-
dc.date.accessioned2019-04-10T19:31:55Z-
dc.date.available2019-04-10T19:31:55Z-
dc.date.issued2012-11en_US
dc.identifier.citationHartman, 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:10.1088/0004-6256/144/5/139en_US
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr17x3m-
dc.description.abstractWe 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.en_US
dc.language.isoen_USen_US
dc.relation.ispartofAstronomical Journalen_US
dc.rightsFinal published version. This is an open access article.en_US
dc.titleHAT-P-39b-HAT-P-41b: Three Highly Inflated Transiting Hot Jupitersen_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.1088/0004-6256/144/5/139-
dc.date.eissued2012-10-09en_US
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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