{"id":31518,"date":"2022-11-10T18:31:11","date_gmt":"2022-11-10T16:31:11","guid":{"rendered":"https:\/\/karmaka.de\/?p=31518"},"modified":"2022-11-10T18:31:11","modified_gmt":"2022-11-10T16:31:11","slug":"presolar-silicon-carbide-grains-of-types-y-and-z-their-strontium-and-barium-isotopic-compositions-and-stellar-origins","status":"publish","type":"post","link":"https:\/\/karmaka.de\/?p=31518","title":{"rendered":"Presolar silicon carbide grains of types Y and Z: their strontium and barium isotopic compositions and stellar origins"},"content":{"rendered":"\n<p>Nan Liu, Thomas Stephan, Sergio Cristallo, Diego Vescovi, Roberto Gallino, Larry R. Nittler, Conel M. O\u2019 D. Alexander &amp; Andrew M. Davis<\/p>\n\n\n\n<p>The European Physical Journal A, Volume 58, Article number: 216<br>Published: 10 November 2022<\/p>\n\n\n\n<p><a href=\"https:\/\/link.springer.com\/article\/10.1140\/epja\/s10050-022-00838-z\" target=\"_blank\" rel=\"noreferrer noopener\"><strong>LINK<\/strong><\/a><\/p>\n\n\n\n<p class=\"justify-text\">&#8220;We report the Sr and Ba isotopic compositions of 18 presolar SiC grains of types Y (11) and Z (7), rare types commonly argued to have formed in lower-than-solar metallicity asymptotic giant branch (AGB) stars. We find that the Y and Z grains show higher 88Sr\/87Sr and more variable 138Ba\/136Ba ratios than mainstream (MS) grains. According to FRANEC Torino AGB models, the Si, Sr, and Ba isotopic compositions of our Y and Z grains can be consistently explained if the grains came from low-mass AGB stars with 0.15 Z\u2299\u2009\u2264\u2009Z\u2009&lt;\u20091.00 Z\u2299, in which the 13C neutron exposure for the slow neutron-capture process is greatly reduced with respect to that required by MS grains for a 1.0 Z\u2299 AGB star. This scenario is in line with the previous finding based on Ti isotopes, but it fails to explain the indistinguishable Mo isotopic compositions of MS, Y, and Z grains.&#8221;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Nan Liu, Thomas Stephan, Sergio Cristallo, Diego Vescovi, Roberto Gallino, Larry R. Nittler, Conel M. O\u2019 D. Alexander &amp; Andrew M. Davis The European Physical Journal A, Volume 58, Article number: 216Published: 10 November 2022&#8230;<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[76],"tags":[627,6399,3855,1084,1853,539,2885],"_links":{"self":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/31518"}],"collection":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=31518"}],"version-history":[{"count":1,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/31518\/revisions"}],"predecessor-version":[{"id":31519,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/31518\/revisions\/31519"}],"wp:attachment":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=31518"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=31518"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=31518"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}