论文标题

WASP调查的两个过渡热木星:黄蜂150b和WASP-176B

Two transiting hot Jupiters from the WASP survey: WASP-150b and WASP-176b

论文作者

Cooke, Benjamin F., Pollacco, Don, Almleaky, Y., Barkaoui, K., Benkhaldoun, Z., Blake, James A., Bouchy, François, Boumis, Panos, Brown, D. J. A., Bruni, Ivan, Burdanov, A., Cameron, Andrew Collier, Chote, Paul, Daassou, A., D'ago, Giuseppe, Dalal, Shweta, Damasso, Mario, Delrez, L., Doyle, A. P., Ducrot, E., Gillon, M., Hébrard, G., Hellier, C., Henning, Thomas, Jehin, E., Kiefer, Flavien, King, George W., Liakos, Alexios, Lopez, Théo, Mancini, Luigi, Mardling, Rosemary, Maxted, P. F. L., McCormac, James, Murray, C., Nielsen, Louise D., Osborn, Hugh, Palle, E., Pepe, Francesco, Pozuelos, F. J., Prieto-Arranz, J., Queloz, D., Schanche, Nicole, Ségransan, Damien, Smalley, Barry, Southworth, John, Thompson, S., Turner, Oliver, Udry, Stéphane, Velasco, S., West, Richard, Wheatley, Pete, Alikakos, John

论文摘要

我们报告了WASP-150b和WASP-176B的两种过渡性系外行星的发现。 WASP-150b是一个偏心($ e $ = 0.38)的热木星,在5.6天的轨道上,左右$ v $ = 12.03,F8主序列主机。主机星的质量和半径为1.4 $ \ rm m _ {\ odot} $和1.7 $ \ rm r _ {\ odot} $。 WASP-150b的质量和半径为8.5 $ \ rm m_j $,1.1 $ \ rm r_j $,导致较大的行星散装密度为6.4 $ \ rmρ_j$。 WASP-150b被发现为$ \ sim3 $ gyr old,远低于其圆形时间尺度,支持地球的怪异性质。 WASP-176B是一个热门木星星球,在3.9天的轨道上,$ V $ = 12.01,F9次巨头主机。主机星的质量和半径为1.3 $ \ rm m _ {\ odot} $和1.9 $ \ rm r _ {\ odot} $。 WASP-176B的质量和半径为0.86 $ \ rm m_j $和1.5 $ \ rm r_j $,导致行星散装密度为0.23 $ \ rmρ_j$。

We report the discovery of two transiting exoplanets from the WASP survey, WASP-150b and WASP-176b. WASP-150b is an eccentric ($e$ = 0.38) hot Jupiter on a 5.6 day orbit around a $V$ = 12.03, F8 main-sequence host. The host star has a mass and radius of 1.4 $\rm M_{\odot}$ and 1.7 $\rm R_{\odot}$ respectively. WASP-150b has a mass and radius of 8.5 $\rm M_J$ and 1.1 $\rm R_J$, leading to a large planetary bulk density of 6.4 $\rm ρ_J$. WASP-150b is found to be $\sim3$ Gyr old, well below its circularisation timescale, supporting the eccentric nature of the planet. WASP-176b is a hot Jupiter planet on a 3.9 day orbit around a $V$ = 12.01, F9 sub-giant host. The host star has a mass and radius of 1.3 $\rm M_{\odot}$ and 1.9 $\rm R_{\odot}$. WASP-176b has a mass and radius of 0.86 $\rm M_J$ and 1.5 $\rm R_J$ respectively, leading to a planetary bulk density of 0.23 $\rm ρ_J$.

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