论文信息 - HAT-P-34b–HAT-P-37b: FOUR TRANSITING PLANETS MORE MASSIVE THAN JUPITER ORBITING MODERATELY BRIGHT STARS - 字舞流文

HAT-P-34b–HAT-P-37b: FOUR TRANSITING PLANETS MORE MASSIVE THAN JUPITER ORBITING MODERATELY BRIGHT STARS

We report the discovery of four transiting extrasolar planets (HAT-P-34b–HAT-P-37b) with masses ranging from 1.05 to 3.33 M_J and periods from 1.33 to 5.45 days. These planets orbit relatively bright F and G dwarf stars (from V = 10.16 to V = 13.2). Of particular interest is HAT-P-34b which is moderately massive (3.33 M_J), has a high eccentricity of e = 0.441 ± 0.032 at a period of P = 5.452654 ± 0.000016 days, and shows hints of an outer component. The other three planets have properties that are typical of hot Jupiters.

Tokyo Institute of Technology | Z. Csubry | UC Berkeley | Planetary Sciences | Caltech | Harvard-Smithsonian Center for Astrophysics | G. Fur'esz | D. W. Latham | A. Bieryla | Astronomy Department | R. W. Noyes | J. D. Hartman | D. O. Astronomy | Avi Shporer | M. Everett | L. Buchhave | D. Latham | D. Sasselov | G. Marcy | A. Howard | S. Quinn | G. Torres | A. Bieryla | G. Esquerdo | Niels Bohr Institute | U. Copenhagen | D. O. Earth | P. Sciences | R. Stefanik | B. Sato | J. Johnson | Lcogt | R. Noyes | J. Hartman | Yale | D. Fischer | A. Department | G. Bakos | A. W. Howard | G. Torres | D. A. Fischer | J. A. Johnson | G. W. Marcy | D. D. Sasselov | R. P. Stefanik | G. A. Esquerdo | Konkoly Observatory | Department of Astronomy | Z. Csubry | K. Penev | J. L'az'ar | I. Papp | P. University | K. Observatory | Hungarian Astronomical Association | Uc Berkeley | Department of Astrophysics | B. B'eky | K. Penev | A. Shporer | L. A. Buchhave | M. Everett | T. Szklen'ar | J. L'az'ar | I. Papp | B. Sato | G. 'A. Bakos | Princeton University | S. Quinn | G. Kov'acs | LCOGT | G. Kov'acs | G. Fur'esz | B. B'eky | T. Szklen'ar | Department of Earth | P. S'ari Department of Astrophysical Sciences | U. of Copenhagen | Dep. of Astrophysics | H. C. F. Astrophysics | D. O. Astrophysics

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