{"provider_name":"Hatena Blog","image_url":null,"title":"astro-ph","blog_title":"\u30cb\u30ef\u30c8\u30ea\u306e\u305f\u307e\u3054","blog_url":"https://niwanoniwatori.hateblo.jp/","height":"190","version":"1.0","html":"<iframe src=\"https://hatenablog-parts.com/embed?url=https%3A%2F%2Fniwanoniwatori.hateblo.jp%2Fentry%2F20130801%2F1375339348\" 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","url":"https://niwanoniwatori.hateblo.jp/entry/20130801/1375339348","width":"100%","description":"Accurate determination of accretion and photospheric parameters in Young Stellar Objects: the case of two candidate old disks in the Orion Nebula Cluster C. F. Manara (1), G. Beccari (1), N. Da Rio (2), G. De Marchi (2), A. Natta (3,4), L. Ricci (5), M. Robberto (6), L. Testi (1,3,7) ((1) ESO-Garchi\u2026","published":"2013-08-01 15:42:28","type":"rich","author_url":"https://blog.hatena.ne.jp/fd_lover24sue/","author_name":"fd_lover24sue","categories":["\u5929\u6587/\u5b87\u5b99"]}