{"id":188,"date":"2014-02-05T15:09:28","date_gmt":"2014-02-05T06:09:28","guid":{"rendered":"http:\/\/guas-astronomy.jp\/weblog\/?p=188"},"modified":"2016-06-16T11:34:31","modified_gmt":"2016-06-16T02:34:31","slug":"vera-observatons-of-sio-masers-toward-symbiotic-star-r-aquarii-determination-of-orbital-parameters-etc","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=188","title":{"rendered":"VERA observatons of SiO masers toward Symbiotic star R Aquarii &#8211; Determination of orbital parameters etc."},"content":{"rendered":"<p>[Speaker 1]<br \/>\nMin Cheul Hong  D2, SOKENDAI, Mitaka\uff08supervisor : Mareki Honma\uff09<br \/>\n[Title]<br \/>\nVERA observatons of SiO masers toward Symbiotic star R Aquarii &#8211; Determination of orbital parameters<br \/>\n[Abstract]<br \/>\nSymbiotic stars are now generally understood as binary systems comprising a cool late-type star and a hot compact companion.<br \/>\nInteracting between the components presents a good laboratory for studying variety of physical processes, and their study gives important implications for the binary evolution.<br \/>\nR Aquarii (R Aqr) is one of the closest and most studied symbiotic star, but its orbital parameters are still under debated.<br \/>\nIn order to extract the orbital parameters, we have been observing the R Aqr system of the SiO maser with the VERA (VLBI Exploration of Radio Astrometry) which can allows us to conduct precise astrometry of the maser sources.<br \/>\nHere, I will report observational results of the preliminary orbital parameters for R Aqr system. <\/p>\n<p>[Speaker 2]<br \/>\nOnitsuka Masahiro  M2, SOKENDAI, Mitaka\uff08supervisor : Tomonori Usuda\uff09<br \/>\n[Title]<br \/>\nInfrared Transit Observations of the Very Young Hot Jupiter CVSO30b<br \/>\n[Abstract]<br \/>\n&#8211;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker 1] Min Cheul Hong D2, SOKENDAI, Mitaka\uff08supervisor : Mareki Honma\uff09 [Title] VERA observatons of SiO mas [&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-188","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\/188","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=188"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/188\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=188"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=188"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=188"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}