{"title":"astro-ph","url":"https://niwanoniwatori.hateblo.jp/entry/20120222/1329911575","categories":["\u5929\u6587/\u5b87\u5b99"],"html":"<iframe src=\"https://hatenablog-parts.com/embed?url=https%3A%2F%2Fniwanoniwatori.hateblo.jp%2Fentry%2F20120222%2F1329911575\" title=\"astro-ph - \u30cb\u30ef\u30c8\u30ea\u306e\u305f\u307e\u3054\" class=\"embed-card embed-blogcard\" scrolling=\"no\" frameborder=\"0\" style=\"display: block; width: 100%; height: 190px; max-width: 500px; margin: 10px 0px;\"></iframe>","provider_url":"https://hatena.blog","provider_name":"Hatena Blog","author_name":"fd_lover24sue","type":"rich","width":"100%","height":"190","version":"1.0","description":"\u30bc\u30df\u3067\u7d39\u4ecb\u3055\u308c\u305f\u3082\u306e\u306e\u30e1\u30e2\u3002 Evidence for enhanced chromospheric Ca II H & K emission in stars with close-in extrasolar planets Tereza Krejcova, Jan Budaj \u60d1\u661f\u304c\u6052\u661f\u306e\u975e\u5e38\u306b\u8fd1\u304f\u3092\u516c\u8ee2\u3057\u3066\u3044\u308b\u3068\u4e3b\u661f\u306e\u6d3b\u52d5\u6027\u304c\u6d3b\u767a\u306b\u306a\u308a\u5f69\u5c64\u306eCaII\u8f1d\u7dda\u304c\u5f37\u304f\u306a\u308b\u3068\u3044\u3046\u3082\u306e\u3002\u305f\u3060\u3001\u3053\u306eCaII\u306e\u5f37\u3055\u306f\u5e74\u9f62\u306b\u3082\u4f9d\u5b58\u3059\u308b\u3082\u306e\u306a\u306e\u3067\u4e3b\u661f\u306e\u30b5\u30f3\u30d7\u30eb\u30bb\u30ec\u30af\u30b7\u30e7\u30f3\u304c\u6c17\u306b\u306a\u308b\u3002 http://jp.arxiv.org/abs/1202.3623 Orbital characterization of \u2026","blog_title":"\u30cb\u30ef\u30c8\u30ea\u306e\u305f\u307e\u3054","blog_url":"https://niwanoniwatori.hateblo.jp/","author_url":"https://blog.hatena.ne.jp/fd_lover24sue/","image_url":null,"published":"2012-02-22 20:52:55"}