Kepler-6b: A TRANSITING HOT JUPITER ORBITING A METAL-RICH STAR

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Kepler-6b : A TRANSITING HOT JUPITER ORBITING A METAL-RICH STAR. / Dunham..[et al.], Edward W.; Borucki, W. J.; Koch, D. G.; Buchhave, Lars C. Astrup.

In: Astrophysical Journal Letters, Vol. 713, No. 2, 20.04.2010, p. L136-L139.

Research output: Contribution to journal › Journal article › Research › peer-review

Harvard

Dunham..[et al.], EW, Borucki, WJ, Koch, DG & Buchhave, LCA 2010, 'Kepler-6b: A TRANSITING HOT JUPITER ORBITING A METAL-RICH STAR', Astrophysical Journal Letters, vol. 713, no. 2, pp. L136-L139. https://doi.org/10.1088/2041-8205/713/2/L136

APA

Dunham..[et al.], E. W., Borucki, W. J., Koch, D. G., & Buchhave, L. C. A. (2010). Kepler-6b: A TRANSITING HOT JUPITER ORBITING A METAL-RICH STAR. Astrophysical Journal Letters, 713(2), L136-L139. https://doi.org/10.1088/2041-8205/713/2/L136

Vancouver

Dunham..[et al.] EW, Borucki WJ, Koch DG, Buchhave LCA. Kepler-6b: A TRANSITING HOT JUPITER ORBITING A METAL-RICH STAR. Astrophysical Journal Letters. 2010 Apr 20;713(2):L136-L139. https://doi.org/10.1088/2041-8205/713/2/L136

Author

Dunham..[et al.], Edward W. ; Borucki, W. J. ; Koch, D. G. ; Buchhave, Lars C. Astrup. / Kepler-6b : A TRANSITING HOT JUPITER ORBITING A METAL-RICH STAR. In: Astrophysical Journal Letters. 2010 ; Vol. 713, No. 2. pp. L136-L139.

Bibtex

@article{fd949b776ff744139ce4a78b3844ffce,
title = "Kepler-6b: A TRANSITING HOT JUPITER ORBITING A METAL-RICH STAR",
abstract = "We announce the discovery of Kepler-6b, a transiting hot Jupiter orbiting a star with unusually high metallicity, . The planet's mass is about 2/3 that of Jupiter, M P = 0.67 M J, and the radius is 30% larger than that of Jupiter, R P = 1.32 R J, resulting in a density of ¿P = 0.35 g cm–3, a fairly typical value for such a planet. The orbital period is P = 3.235 days. The host star is both more massive than the Sun, M = 1.21 M , and larger than the Sun, R = 1.39 R ",
author = "{Dunham..[et al.]}, {Edward W.} and Borucki, {W. J.} and Koch, {D. G.} and Buchhave, {Lars C. Astrup}",
year = "2010",
month = apr,
day = "20",
doi = "10.1088/2041-8205/713/2/L136",
language = "English",
volume = "713",
pages = "L136--L139",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing, Inc",
number = "2",

}

RIS

TY - JOUR

T1 - Kepler-6b

T2 - A TRANSITING HOT JUPITER ORBITING A METAL-RICH STAR

AU - Dunham..[et al.], Edward W.

AU - Borucki, W. J.

AU - Koch, D. G.

AU - Buchhave, Lars C. Astrup

PY - 2010/4/20

Y1 - 2010/4/20

N2 - We announce the discovery of Kepler-6b, a transiting hot Jupiter orbiting a star with unusually high metallicity, . The planet's mass is about 2/3 that of Jupiter, M P = 0.67 M J, and the radius is 30% larger than that of Jupiter, R P = 1.32 R J, resulting in a density of ¿P = 0.35 g cm–3, a fairly typical value for such a planet. The orbital period is P = 3.235 days. The host star is both more massive than the Sun, M = 1.21 M , and larger than the Sun, R = 1.39 R

AB - We announce the discovery of Kepler-6b, a transiting hot Jupiter orbiting a star with unusually high metallicity, . The planet's mass is about 2/3 that of Jupiter, M P = 0.67 M J, and the radius is 30% larger than that of Jupiter, R P = 1.32 R J, resulting in a density of ¿P = 0.35 g cm–3, a fairly typical value for such a planet. The orbital period is P = 3.235 days. The host star is both more massive than the Sun, M = 1.21 M , and larger than the Sun, R = 1.39 R

U2 - 10.1088/2041-8205/713/2/L136

DO - 10.1088/2041-8205/713/2/L136

M3 - Journal article

VL - 713

SP - L136-L139

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 2

ER -

ID: 32928483