Interferometric diameters of five evolved intermediate-mass planet-hosting stars measured with PAVO at the CHARA Array
Interferometric diameters of five evolved intermediate-mass planet-hosting stars measured with PAVO at the CHARA Array
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DOI:
10.1093/mnras/sty898
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发表时间:
2018-04
影响因子:
4.8
通讯作者:
T. White;T. White;T. White;D. Huber;A. Mann;A. Mann;L. Casagrande;S. Grunblatt;A. B. Justesen;V. S. Aguirre;T. Bedding;T. Bedding;M. Ireland;G. Schaefer;P. Tuthill
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文献类型:
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作者:
T. White;T. White;T. White;D. Huber;A. Mann;A. Mann;L. Casagrande;S. Grunblatt;A. B. Justesen;V. S. Aguirre;T. Bedding;T. Bedding;M. Ireland;G. Schaefer;P. Tuthill
Funding for the Stellar Astrophysics Centre is provided by The Danish National Research Foundation. The research was supported by the ASTERISK project (ASTERoseismic Investigations with SONG and Kepler) funded by the European Research Council (Grant agreement no.: 267864). TRW and VSA acknowledge the support of the Villum Foundation (research grant 10118). DH acknowledges support by the Australian Research Council’s Discovery Projects funding scheme (project number DE140101364) and support by the NASA Grant NNX14AB92G issued through the Kepler Participating Scientist Program. LC is supported by the Australian Research Council Future Fellowship FT160100402. MJI was supported by the Australian Research Council Future Fellowship FT130100235. Parts of this research were conducted by the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013.