HAT-P-6b:: A hot jupiter transiting a bright F star

被引：64

作者：

Noyes, R. W. ^{[1
]}

Bakos, G. A. ^{[1
]}

Torres, G. ^{[1
]}

Pal, A. ^{[1
,2
]}

Kovacs, Geza ^{[3
]}

Latham, D. W. ^{[1
]}

Fernandez, J. M. ^{[1
]}

Fischer, D. A. ^{[4
]}

Butler, R. P. ^{[5
]}

Marcy, G. W. ^{[6
]}

Sipocz, B. ^{[1
,2
]}

Esquerdo, G. A. ^{[1
]}

Kovacs, Gabor ^{[1
]}

Sasselov, D. D. ^{[1
]}

Sato, B. ^{[7
]}

Stefanik, R. ^{[1
]}

Holman, M. ^{[1
]}

Lazar, J. ^{[8
]}

Papp, I. ^{[8
]}

Sari, P. ^{[8
]}

机构：

[1] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA

[2] Eotvos Lorand Univ, Dept Astron, Budapest, Hungary

[3] Konkoly Observ Budapest, Budapest, Hungary

[4] San Francisco State Univ, Dept Phys & Astron, San Francisco, CA 94132 USA

[5] Carnegie Inst Washington, Dept Terr Magnetism, Washington, DC 20015 USA

[6] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA

[7] Tokyo Inst Technol, Tokyo 152, Japan

[8] Hungarian Astron Assoc, Budapest, Hungary

来源：

ASTROPHYSICAL JOURNAL LETTERS | 2008年 / 673卷 / 01期

关键词：

planetary systems; stars; individual; (GSC; 03239-00992; HAT-P-6);

D O I：

10.1086/527358

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In the ongoing HATNet survey we have detected a giant planet, with radius 1.33 +/- 0.06 R(Jup) and mass 1.06 +/- 0.12 M(Jup), transiting the bright (V = 10.5) star GSC 03239-00992. The planet is in a circular orbit with period days and midtransit epoch 2,454,035.67575 +/- 0.00028 ( HJD). The parent star is 3.852985 +/- 0.000005 a late F star with mass, radius, 1.29 +/- 0.06 M(circle dot), radius 1.46 +/- 0.06 R(circle dot), T(eff) similar to 6570 +/- 80 K [Fe/H] = -0.13 +/- 0.08, and age similar to 2.3(-0.7)(+0.5) Gyr. With this radius and mass, HAT-P-6b has somewhat larger radius than theoretically expected. We describe the observations and their analysis to determine physical properties of the HAT- P- 6 system, and briefly discuss some implications of this finding.

引用

页码：L79 / L82

页数：4

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