{"id":1049,"date":"2022-06-15T09:06:30","date_gmt":"2022-06-15T09:06:30","guid":{"rendered":"http:\/\/www.astro.me.uk\/?p=1049"},"modified":"2022-06-15T09:10:04","modified_gmt":"2022-06-15T09:10:04","slug":"new-paper-accepted-by-royal-astronomical-society","status":"publish","type":"post","link":"https:\/\/www.astro.me.uk\/?p=1049","title":{"rendered":"New paper accepted by Royal Astronomical Society."},"content":{"rendered":"\n<p>Now loaded on arXiv.org  Cornell University Archive.<\/p>\n\n\n\n<ol><li><a href=\"https:\/\/arxiv.org\/abs\/2206.06919\">arXiv:2206.06919<\/a>\u00a0\u00a0[<a href=\"https:\/\/arxiv.org\/pdf\/2206.06919\">pdf<\/a>,\u00a0<a href=\"https:\/\/arxiv.org\/ps\/2206.06919\">ps<\/a>,\u00a0<a href=\"https:\/\/arxiv.org\/format\/2206.06919\">other<\/a>]\u00a0\u00a0astro-ph.SR\u00a0astro-ph.EPEclipse timing variations in post-common envelope binaries: Are they a reliable indicator of circumbinary companions?<\/li><li><strong>Authors:<\/strong>\u00a0<a href=\"https:\/\/arxiv.org\/search\/?searchtype=author&amp;query=Pulley%2C+D\">D. Pulley<\/a>,\u00a0<a href=\"https:\/\/arxiv.org\/search\/?searchtype=author&amp;query=Sharp%2C+I+D\">I. D. Sharp<\/a>,\u00a0<a href=\"https:\/\/arxiv.org\/search\/?searchtype=author&amp;query=Mallett%2C+J\">J. Mallett<\/a>,\u00a0<a href=\"https:\/\/arxiv.org\/search\/?searchtype=author&amp;query=von+Harrach%2C+S\">S. von Harrach<\/a><\/li><li>Abstract:\u00a0Post-common envelope binary systems evolve when matter is transferred from the primary star at a rate that cannot be accommodated by its secondary companion. A common envelope forms which is subsequently ejected resulting in a system with a binary period frequently between 2 and 3 hours. Where circumbinary companions are predicted, it remains unclear whether they form before or after the common en\u2026<\/li><li>\u00a0<a>\u25bd More<\/a>Submitted\u00a014 June, 2022;\u00a0originally announced\u00a0June 2022.Comments:\u00a016 pages, 8 figures, 7 binary systems and 163 observations<\/li><\/ol>\n\n\n\n<p><\/p>\n","protected":false},"excerpt":{"rendered":"\n<p>Now loaded on arXiv.org Cornell University Archive.<\/p>\n<p> arXiv:2206.06919 [pdf, ps, other] astro-ph.SR astro-ph.EPEclipse timing variations in post-common envelope binaries: Are they a reliable indicator of circumbinary companions?Authors: D. Pulley, I. D. Sharp, J. Mallett, S. von HarrachAbstract: Post-common envelope binary systems evolve when matter is transferred from the primary star at a rate that [&#8230;]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[1],"tags":[],"_links":{"self":[{"href":"https:\/\/www.astro.me.uk\/index.php?rest_route=\/wp\/v2\/posts\/1049"}],"collection":[{"href":"https:\/\/www.astro.me.uk\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.astro.me.uk\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.astro.me.uk\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/www.astro.me.uk\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=1049"}],"version-history":[{"count":3,"href":"https:\/\/www.astro.me.uk\/index.php?rest_route=\/wp\/v2\/posts\/1049\/revisions"}],"predecessor-version":[{"id":1052,"href":"https:\/\/www.astro.me.uk\/index.php?rest_route=\/wp\/v2\/posts\/1049\/revisions\/1052"}],"wp:attachment":[{"href":"https:\/\/www.astro.me.uk\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=1049"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.astro.me.uk\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=1049"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.astro.me.uk\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=1049"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}