期刊
ASTRONOMICAL JOURNAL
卷 133, 期 4, 页码 1828-1835出版社
IOP PUBLISHING LTD
DOI: 10.1086/512159
关键词
planetary systems; planetary systems : formation; stars : individual (HD 189733); stars : rotation
We present photometry of HD 189733 during eight transits of its close-in giant planet, and out-of-transit photometry spanning 2 yr. Using the transit photometry, we determine the stellar and planetary radii and the photometric ephemeris. Outside of transits, there are quasi-periodic flux variations with a 13.4 day period that we attribute to stellar rotation. In combination with previous results, we derive upper limits on the orbital eccentricity and on the true angle between the stellar rotation axis and planetary orbit (as opposed to the angle between the projections of those axes on the sky).
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