{"image_url":null,"title":"astro-ph","version":"1.0","provider_name":"Hatena Blog","html":"<iframe src=\"https://hatenablog-parts.com/embed?url=https%3A%2F%2Fniwanoniwatori.hateblo.jp%2Fentry%2F20130628%2F1372400725\" 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>","type":"rich","blog_url":"https://niwanoniwatori.hateblo.jp/","blog_title":"\u30cb\u30ef\u30c8\u30ea\u306e\u305f\u307e\u3054","height":"190","author_url":"https://blog.hatena.ne.jp/fd_lover24sue/","author_name":"fd_lover24sue","categories":["\u5929\u6587/\u5b87\u5b99"],"provider_url":"https://hatena.blog","description":"Statistical Properties of Brown Dwarf Companions: Implications for Different Formation Mechanisms Bo Ma, Jian Ge \u4f34\u661f\u578b\u306e\u8910\u8272\u77ee\u661f\u306e\u7269\u7406\u91cf\u3092\u6bd4\u8f03\u3059\u308b\u306843\u6728\u661f\u8cea\u91cf\u3067\u533a\u5207\u308b\u3068\u96e2\u5fc3\u7387\u306a\u3069\u306b\u6709\u610f\u306a\u9055\u3044\u304c\u3042\u308a\u300143\u4ee5\u4e0b\u3067\u306f\u60d1\u661f\u7684\u306b\u5f62\u6210\u3055\u308c\u300143\u4ee5\u4e0a\u3067\u306f\u4f34\u661f\u7684\u306b\u5f62\u6210\u3055\u308c\u308b\u306e\u3067\u306f\u3068\u3044\u3046\u3082\u306e http://jp.arxiv.org/abs/1303.6442","published":"2013-06-28 15:25:25","width":"100%","url":"https://niwanoniwatori.hateblo.jp/entry/20130628/1372400725"}