{"id":908,"date":"2018-07-11T14:48:13","date_gmt":"2018-07-11T05:48:13","guid":{"rendered":"https:\/\/guas-astronomy.jp\/weblog\/?p=908"},"modified":"2019-07-08T15:50:32","modified_gmt":"2019-07-08T06:50:32","slug":"radiation-hydrodynamics-simulations-of-photoevaporation-of-protoplanetary-disks-metallicity-dependence-of-uv-and-x-ray-photoevaporation","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=908","title":{"rendered":"Tensile Strength of Porous Dust Aggregates\/Review of High-Resolution Near-IR Spectroscopy of M-dwarfs with CARMENES"},"content":{"rendered":"<p>[Speaker 1]<br \/>\nMisako Tatsuuma,<br \/>\nUniversity of Tokyo D1<br \/>\n(Supervisor: Eiichiro Kokubo)<\/p>\n<p>[Title 1]<br \/>\nTensile Strength of Porous Dust Aggregates<\/p>\n<p>[Speaker 2]<br \/>\nHiroyuki Tako ISHIKAWA,<br \/>\nSOKENDAI 3rd year (D1)<br \/>\n(Supervisor: Tomonori Usuda,Saeko Hayashi,Takayuki Kotani)<\/p>\n<p>[Title 2]<br \/>\nReview of High-Resolution Near-IR Spectroscopy of M-dwarfs with CARMENES<\/p>\n<p>[Abstract 2]<br \/>\nI am now attempting to establish the abundance analysis of late-M dwarfs by using Subaru-IRD data. In Europe, the CARMENES group also performs the high-resolution near-infrared spectroscopy on M dwarfs in search of exoplanets. In this talk, I will review the papers written by the CARMENES group, especially those related to the stellar characterization (mainly, V. M. Passegger et al. 2018, A&amp;A).<br \/>\nPlease note that the presenter information posted here is not necessarily listed in order of presentation.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker 1] Misako Tatsuuma, University of Tokyo D1 (Supervisor: Eiichiro Kokubo) [Title 1] Tensile Strength o [&hellip;]<\/p>\n","protected":false},"author":2,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[6,5],"tags":[],"class_list":["post-908","post","type-post","status-publish","format-standard","hentry","category-6","category-5"],"_links":{"self":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/908","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=908"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/908\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=908"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=908"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=908"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}