HAT-P-39b-HAT-P-41b: three highly inflated transiting hot Jupiters

J. D. Hartman; G. Á. Bakos; B. Béky; G. Torres; D. W. Latham; Z. Csubry; K. Penev; A. Shporer; B. J. Fulton; Lars A. Buchhave; J. A. Johnson; A. W. Howard; G. W. Marcy; D. A. Fischer; G. Kovács; R. W. Noyes; G. A. Esquerdo; M. Everett; T. Szklenár; S. N. Quinn; A. Bieryla; R. P. Knox; P. Hinz; D. D. Sasselov; G. Fűrész; R. P. Stefanik; J. Lázár; I. Papp; P. Sári

doi:10.1088/0004-6256/144/5/139

HAT-P-39b-HAT-P-41b: three highly inflated transiting hot Jupiters

J. D. Hartman, G. Á. Bakos, B. Béky, G. Torres, D. W. Latham, Z. Csubry, K. Penev, A. Shporer, B. J. Fulton, Lars A. Buchhave, J. A. Johnson, A. W. Howard, G. W. Marcy, D. A. Fischer, G. Kovács, R. W. Noyes, G. A. Esquerdo, M. Everett, T. Szklenár, S. N. QuinnA. Bieryla, R. P. Knox, P. Hinz, D. D. Sasselov, G. Fűrész, R. P. Stefanik, J. Lázár, I. Papp, P. Sári

Astrophysics and Planetary Science

60 Citations (Scopus)

Abstract

We report the discovery of three new transiting extrasolar planets orbiting moderately bright (V = 11.1, 11.7, and12.4) F stars. The planets HAT-P-39b through HAT-P-41b have periods of P = 3.5439days, 4.4572days, and 2.6940days, masses of 0.60M _J,0.62M _J, and 0.80M _J, and radii of 1.57R _J,1.73R _J, and 1.68R _J, respectively. They orbit stars with masses of 1.40M _⊙,1.51M _⊙, and 1.51M _⊙, 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.

Original language	English
Article number	139
Journal	Astronomical Journal
Volume	144
Issue number	5
Number of pages	18
ISSN	0004-6256
DOIs	https://doi.org/10.1088/0004-6256/144/5/139
Publication status	Published - 1 Nov 2012

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Hartman, J. D., Bakos, G. Á., Béky, B., Torres, G., Latham, D. W., Csubry, Z., Penev, K., Shporer, A., Fulton, B. J., Buchhave, L. A., Johnson, J. A., Howard, A. W., Marcy, G. W., Fischer, D. A., Kovács, G., Noyes, R. W., Esquerdo, G. A., Everett, M., Szklenár, T., ... Sári, P. (2012). HAT-P-39b-HAT-P-41b: three highly inflated transiting hot Jupiters. Astronomical Journal, 144(5), [139]. https://doi.org/10.1088/0004-6256/144/5/139

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, Fűrész, G, Stefanik, RP, Lázár, J, Papp, I & Sári, P 2012, 'HAT-P-39b-HAT-P-41b: three highly inflated transiting hot Jupiters', Astronomical Journal, vol. 144, no. 5, 139. https://doi.org/10.1088/0004-6256/144/5/139

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title = "HAT-P-39b-HAT-P-41b: three highly inflated transiting hot Jupiters",

abstract = "We report the discovery of three new transiting extrasolar planets orbiting moderately bright (V = 11.1, 11.7, and12.4) F stars. The planets HAT-P-39b through HAT-P-41b have periods of P = 3.5439days, 4.4572days, and 2.6940days, masses of 0.60M J,0.62M J, and 0.80M J, and radii of 1.57R J,1.73R J, and 1.68R J, respectively. They orbit stars with masses of 1.40M ⊙,1.51M ⊙, and 1.51M ⊙, 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.",

author = "Hartman, {J. D.} and Bakos, {G. {\'A}.} and B. B{\'e}ky and G. Torres and Latham, {D. W.} and Z. Csubry and K. Penev and A. Shporer and Fulton, {B. J.} and Buchhave, {Lars A.} and Johnson, {J. A.} and Howard, {A. W.} and Marcy, {G. W.} and Fischer, {D. A.} and G. Kov{\'a}cs and Noyes, {R. W.} and Esquerdo, {G. A.} and M. Everett and T. Szklen{\'a}r and Quinn, {S. N.} and A. Bieryla and Knox, {R. P.} and P. Hinz and Sasselov, {D. D.} and G. F{\H u}r{\'e}sz and Stefanik, {R. P.} and J. L{\'a}z{\'a}r and I. Papp and P. S{\'a}ri",

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T1 - HAT-P-39b-HAT-P-41b

T2 - three highly inflated transiting hot Jupiters

AU - Hartman, J. D.

AU - Bakos, G. Á.

AU - Béky, B.

AU - Torres, G.

AU - Latham, D. W.

AU - Csubry, Z.

AU - Penev, K.

AU - Shporer, A.

AU - Fulton, B. J.

AU - Buchhave, Lars A.

AU - Johnson, J. A.

AU - Howard, A. W.

AU - Marcy, G. W.

AU - Fischer, D. A.

AU - Kovács, G.

AU - Noyes, R. W.

AU - Esquerdo, G. A.

AU - Everett, M.

AU - Szklenár, T.

AU - Quinn, S. N.

AU - Bieryla, A.

AU - Knox, R. P.

AU - Hinz, P.

AU - Sasselov, D. D.

AU - Fűrész, G.

AU - Stefanik, R. P.

AU - Lázár, J.

AU - Papp, I.

AU - Sári, P.

PY - 2012/11/1

Y1 - 2012/11/1

N2 - We report the discovery of three new transiting extrasolar planets orbiting moderately bright (V = 11.1, 11.7, and12.4) F stars. The planets HAT-P-39b through HAT-P-41b have periods of P = 3.5439days, 4.4572days, and 2.6940days, masses of 0.60M J,0.62M J, and 0.80M J, and radii of 1.57R J,1.73R J, and 1.68R J, respectively. They orbit stars with masses of 1.40M ⊙,1.51M ⊙, and 1.51M ⊙, 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.

AB - We report the discovery of three new transiting extrasolar planets orbiting moderately bright (V = 11.1, 11.7, and12.4) F stars. The planets HAT-P-39b through HAT-P-41b have periods of P = 3.5439days, 4.4572days, and 2.6940days, masses of 0.60M J,0.62M J, and 0.80M J, and radii of 1.57R J,1.73R J, and 1.68R J, respectively. They orbit stars with masses of 1.40M ⊙,1.51M ⊙, and 1.51M ⊙, 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.

U2 - 10.1088/0004-6256/144/5/139

DO - 10.1088/0004-6256/144/5/139

M3 - Journal article

SN - 0004-6256

VL - 144

JO - The Astronomical Journal

JF - The Astronomical Journal

IS - 5

M1 - 139

ER -

HAT-P-39b-HAT-P-41b: three highly inflated transiting hot Jupiters

Abstract

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