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HATS-15b and HATS-16b: Two Massive Planets Transiting Old G Dwarf Stars

Author(s): Ciceri, S; Mancini, L; Henning, T; Bakos, Gaspar Aron; Penev, K; et al

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dc.contributor.authorCiceri, S-
dc.contributor.authorMancini, L-
dc.contributor.authorHenning, T-
dc.contributor.authorBakos, Gaspar Aron-
dc.contributor.authorPenev, K-
dc.contributor.authorBrahm, R-
dc.contributor.authorZhou, G-
dc.contributor.authorHartman, Joel D.-
dc.contributor.authorBayliss, D-
dc.contributor.authorJordán, A.-
dc.contributor.authorCsubry, Zoltan-
dc.contributor.authorde Val-Borro, Miguel-
dc.contributor.authorBhatti, W-
dc.contributor.authorRabus, M-
dc.contributor.authorEspinoza, N-
dc.contributor.authorSuc, V-
dc.contributor.authorSchmidt, B-
dc.contributor.authorNoyes, Robert W.-
dc.contributor.authorHoward, AW-
dc.contributor.authorFulton, BJ-
dc.contributor.authorIsaacson, H-
dc.contributor.authorMarcy, GW-
dc.contributor.authorButler, RP-
dc.contributor.authorArriagada, P-
dc.contributor.authorCrane, JD-
dc.contributor.authorShectman, S-
dc.contributor.authorThompson, I-
dc.contributor.authorTan, TG-
dc.contributor.authorLázár, J.-
dc.contributor.authorPapp, I-
dc.contributor.authorSári, P-
dc.date.accessioned2019-04-10T19:32:17Z-
dc.date.available2019-04-10T19:32:17Z-
dc.date.issued2016-07en_US
dc.identifier.citationCiceri, S, Mancini, L, Henning, T, Bakos, G, Penev, K, Brahm, R, Zhou, G, Hartman, JD, Bayliss, D, Jordán, A, Csubry, Z, de Val-Borro, M, Bhatti, W, Rabus, M, Espinoza, N, Suc, V, Schmidt, B, Noyes, R, Howard, AW, Fulton, BJ, Isaacson, H, Marcy, GW, Butler, RP, Arriagada, P, Crane, JD, Shectman, S, Thompson, I, Tan, TG, Lázár, J, Papp, I, Sari, P. (2016). HATS-15b and HATS-16b: Two Massive Planets Transiting Old G Dwarf Stars. Publications of the Astronomical Society of the Pacific, 128 (074401 - 074401. doi:10.1088/1538-3873/128/965/074401en_US
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr1pt3z-
dc.description.abstractWe report the discovery of HATS-15 b and HATS-16 b, two massive transiting extrasolar planets orbiting evolved (∼10 Gyr) main-sequence stars. The planet HATS-15 b, which is hosted by a G9 V star (V = 14.8 mag), is a hot Jupiter with mass of 2.17 0.15  MJ and radius of 1.105 0.040  RJ, and it completes its orbit in about 1.7 days. HATS-16 b is a very massive hot Jupiter with mass of 3.27 0.19  MJ and radius of 1.30 0.15 ;  RJ it orbits around its G3 V parent star (V = 13.8 mag) in ∼2.7 days. HATS-16 is slightly active and shows a periodic photometric modulation, implying a rotational period of 12 days, which is unexpectedly short given its isochronal age. This fast rotation might be the result of the tidal interaction between the star and its planet.en_US
dc.language.isoen_USen_US
dc.relation.ispartofPublications of the Astronomical Society of the Pacificen_US
dc.rightsFinal published version. This is an open access article.en_US
dc.titleHATS-15b and HATS-16b: Two Massive Planets Transiting Old G Dwarf Starsen_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.1088/1538-3873/128/965/074401-
dc.date.eissued2016-06-10en_US
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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