{"height":"190","type":"rich","author_url":"https://blog.hatena.ne.jp/fd_lover24sue/","version":"1.0","author_name":"fd_lover24sue","url":"https://niwanoniwatori.hateblo.jp/entry/20130730/1375166152","provider_url":"https://hatena.blog","blog_title":"\u30cb\u30ef\u30c8\u30ea\u306e\u305f\u307e\u3054","html":"<iframe src=\"https://hatenablog-parts.com/embed?url=https%3A%2F%2Fniwanoniwatori.hateblo.jp%2Fentry%2F20130730%2F1375166152\" 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>","image_url":null,"width":"100%","provider_name":"Hatena Blog","description":"Spectral and Photometric Diagnostics of Giant Planet Formation Scenarios David S. Spiegel (1, 2), Adam Burrows (2) ((1) Institute for Advanced Study (2) Princeton University) http://xxx.yukawa.kyoto-u.ac.jp/abs/1108.5172","categories":["\u5929\u6587/\u5b87\u5b99"],"title":"astro-ph","blog_url":"https://niwanoniwatori.hateblo.jp/","published":"2013-07-30 15:35:52"}