To refer to this page use:
|Abstract:||We report the discovery of the transiting extrasolar planet HAT-P-49b. The planet transits the bright (V = 10.3) slightly evolved F-star HD 340099 with a mass of 1.54 M⊙and a radius of 1.83 R ⊙ . HAT-P-49b is orbiting one of the 25 brightest stars to host a transiting planet which makes this a favorable candidate for detailed follow-up. This system is an especially strong target for Rossiter-McLaughlin follow-up due to the host star’s fast rotation, 16 km s-1. The planetary companion has a period of 2.6915 days, mass of 1.73 M J, and radius of 1.41 R J. The planetary characteristics are consistent with that of a classical hot Jupiter but we note that this is the fourth most massive star to host a transiting planet with both Mp and Rp well determined. © 2014. The American Astronomical Society. All rights reserved..|
|Electronic Publication Date:||13-Mar-2014|
|Citation:||Bieryla, A, Hartman, JD, Bakos, GA, Bhatti, W, Kovács, G, Boisse, I, Latham, DW, Buchhave, LA, Csubry, Z, Penev, K, De Val-Borro, M, Béky, B, Falco, E, Torres, G, Noyes, RW, Berlind, P, Calkins, MC, Esquerdo, GA, Lázár, J, Papp, I, Sári, P. (2014). HAT-P-49b: A 1.7 M<inf>J</inf> planet transiting a bright 1.5 M⊙F-star. Astronomical Journal, 147 (4), 10.1088/0004-6256/147/4/84|
|Type of Material:||Journal Article|
|Journal/Proceeding Title:||Astronomical Journal|
|Version:||Final published version. Article is made available in OAR by the publisher's permission or policy.|
Items in OAR@Princeton are protected by copyright, with all rights reserved, unless otherwise indicated.