{"id":127,"date":"2019-11-22T19:39:34","date_gmt":"2019-11-22T17:39:34","guid":{"rendered":"http:\/\/www.issibern.ch\/teams\/chemabundism\/?page_id=127"},"modified":"2019-11-22T19:39:34","modified_gmt":"2019-11-22T17:39:34","slug":"publications","status":"publish","type":"page","link":"https:\/\/www.issibern.ch\/teams\/chemabundism\/publications\/","title":{"rendered":"Publications"},"content":{"rendered":"<p style=\"text-align: justify\"><span style=\"font-weight: 400\">The discussions held in ISSI and ISSI-BJ and the support from ISSI\/ISSI-BJ are acknowledged in the following refereed publications:<\/span><\/p>\n<ul>\n<li style=\"font-weight: 400;text-align: justify\"><b>Kroupa P., Jerabkova T.,<\/b><span style=\"font-weight: 400\"> \u201c<\/span><i><span style=\"font-weight: 400\">The Salpeter IMF and its descendants\u201d<\/span><\/i><span style=\"font-weight: 400\">, 2019, Nat. Astr., 3, 482<\/span><\/li>\n<li style=\"font-weight: 400;text-align: justify\"><b>Yan Z., Jerabkova T., Kroupa P.,<\/b><span style=\"font-weight: 400\"> Vazdekis A., <\/span><i><span style=\"font-weight: 400\">\u201cChemical evolution of elliptical galaxies with a variable IMF. A publicly available code\u201d<\/span><\/i><span style=\"font-weight: 400\">, 2019, A&amp;A, 629, A93<\/span><\/li>\n<li style=\"font-weight: 400;text-align: justify\"><b>Romano D., Matteucci F., Zhang Z.-Y., Ivison R., Ventura P.,<\/b> <i><span style=\"font-weight: 400\">\u201cThe evolution of CNO isotopes: the impact of massive stellar rotators\u201d<\/span><\/i><span style=\"font-weight: 400\">, 2019, MNRAS, 490, 2838<\/span><\/li>\n<li style=\"font-weight: 400;text-align: justify\"><b>Yan Z., Jerabkova T., Kroupa P.,<\/b> <i><span style=\"font-weight: 400\">\u201cThe star formation timescale of elliptical galaxies. Fitting [Mg\/Fe] and total metallicity simultaneously\u201d<\/span><\/i><span style=\"font-weight: 400\">, 2019, A&amp;A, 632, A110<\/span><\/li>\n<li><span style=\"font-weight: 400\">Li F., <\/span><b>Wang J.,<\/b><span style=\"font-weight: 400\"> &#8230;, <\/span><b>Zhang Z.-Y.,<\/b><span style=\"font-weight: 400\"> &#8230;, <\/span><i><span style=\"font-weight: 400\">\u201cIsotopologues of dense gas tracers in nearby infrared bright galaxies\u201d<\/span><\/i><span style=\"font-weight: 400\">, 2020, MNRAS, 494, 1095<\/span><\/li>\n<li><b>Yan Z., Jerabkova T., Kroupa P.,<\/b> <i><span style=\"font-weight: 400\">\u201cChemical evolution of ultra-faint dwarf galaxies in the self-consistently calculated integrated galactic IMF theory\u201d<\/span><\/i><span style=\"font-weight: 400\">, 2020, A&amp;A, 637, A68<\/span><\/li>\n<li style=\"font-weight: 400;text-align: justify\"><span style=\"font-weight: 400\">Zhang J. S., \u2026, <\/span><b>Romano D., Zhang Z.-Y., Wang J. Z.,<\/b><span style=\"font-weight: 400\"> \u2026, <\/span><i><span style=\"font-weight: 400\">\u201cA systematic observational study on Galactic interstellar ratio <\/span><\/i><sup><i><span style=\"font-weight: 400\">18<\/span><\/i><\/sup><i><span style=\"font-weight: 400\">O\/<\/span><\/i><sup><i><span style=\"font-weight: 400\">17<\/span><\/i><\/sup><i><span style=\"font-weight: 400\">O. I. C<\/span><\/i><sup><i><span style=\"font-weight: 400\">18<\/span><\/i><\/sup><i><span style=\"font-weight: 400\">O and C<\/span><\/i><sup><i><span style=\"font-weight: 400\">17<\/span><\/i><\/sup><i><span style=\"font-weight: 400\">O J = 1\u22120 data analysis\u201d<\/span><\/i><span style=\"font-weight: 400\">, 2020, ApJS, 249, 6<\/span><\/li>\n<li><span style=\"color: #333333\"><b>Romano D., <span style=\"font-weight: 400\">Franchini M., Grisoni V., Spitoni E., <\/span><\/b><strong>Matteucci F.,<\/strong> <span style=\"font-weight: 400\">Morossi C.,<\/span>\u00a0<em><span style=\"font-weight: 400\">\u201c<\/span>T<\/em><i><span style=\"font-weight: 400\">he variation of carbon abundance in galaxies and its implications\u201d<\/span><\/i><span style=\"font-weight: 400\">, 2020, A&amp;A, 639, A37<\/span><\/span><\/li>\n<li style=\"font-weight: 400;text-align: justify\"><span style=\"font-weight: 400;color: #333333\">Mendez-Hernandez H., &#8230;, <strong>Zhang Z.-Y.,<\/strong> &#8230;,\u00a0<i>\u201c<\/i><em>Vales VI: ISM enrichment in star-forming galaxies up to z~0.2 using <sup>12<\/sup>CO(<i>1\u22120<\/i>), <sup>13<\/sup>CO(<i>1\u22120<\/i>) and C<sup>18<\/sup>O(<i>1\u22120<\/i>) line luminosity ratios<i>\u201d<\/i>,\u00a0<\/em>2020, MNRAS, 497, 2771<\/span><\/li>\n<li><span style=\"color: #333333\"><strong>Ventura P., <span style=\"font-weight: 400\">Dell&#8217;Agli F., Lugaro M.,<\/span><\/strong>\u00a0<strong>Romano D., <span style=\"font-weight: 400\">Tailo M., Yag\u00fce A., <span style=\"font-weight: 400;color: #333333\"><i>\u201cGa<em>s and dust from metal-rich AGB stars\u201d,<\/em><\/i>\u00a02020, A&amp;A<\/span><\/span><\/strong><\/span><span style=\"color: #333333\"><strong><span style=\"font-weight: 400\"><span style=\"font-weight: 400;color: #333333\">, 641, A103<\/span><\/span><\/strong><\/span><\/li>\n<li><strong>Xie L.,<\/strong> <span style=\"font-weight: 400;color: #333333\">De Lucia G., Hirschmann M., Fontanot F., <span style=\"color: #333333\"><strong><span style=\"font-weight: 400\"><i>\u201cThe influence of environment on satellite galaxies in the GAEA semi-analytic model<em>\u201d, <\/em><\/i><\/span><\/strong><\/span>2020, MNRAS, 498, 4327<\/span><\/li>\n<li><span style=\"font-weight: 400;color: #333333\">Minelli A., Mucciarelli A.,\u00a0<strong>Romano D.,<\/strong> Bellazzini M., Origlia L., Ferraro F. R., <span style=\"color: #333333\"><strong><span style=\"font-weight: 400\"><i>\u201cA Homogeneous Comparison between the Chemical Composition of the Large Magellanic Cloud and the Sagittarius Dwarf<\/i> Galaxy\u201d<em>,<\/em> 2021, ApJ, 910, 114<\/span><\/strong><\/span><\/span><\/li>\n<li><span style=\"font-weight: 400;color: #333333\">Grisoni V.,\u00a0<strong>Matteucci F., Romano D.,<\/strong> <span style=\"color: #333333\"><strong><span style=\"font-weight: 400\"><i>\u201cNitrogen evolution in the thick disc, thin disc, and bulge of the Galaxy<em>\u201d, <\/em><\/i>2021, MNRAS, 508, 719<\/span><\/strong><\/span><\/span><\/li>\n<li><span style=\"font-weight: 400;color: #333333\">Mucciarelli A., Massari D., Minelli A., <strong>Romano D.,<\/strong> Bellazzini M., Ferraro F. R., <strong>Matteucci F.,<\/strong> Origlia L., <span style=\"color: #333333\"><strong><span style=\"font-weight: 400\"><i>\u201cA relic from a past merger event in the Large Magellanic Cloud<\/i><em>\u201d,<\/em> 2021, Nature Astronomy, 5, 1247<\/span><\/strong><\/span><\/span><\/li>\n<li><span style=\"color: #333333\"><strong>Ventura P., <span style=\"font-weight: 400\">Dell&#8217;Agli F., <\/span><\/strong><strong>Romano D., <span style=\"font-weight: 400\">Tosi S., Limongi M., Chieffi A., Castellani M., Tailo M., Lugaro M., Marini E., Yag\u00fce-Lopez A., <span style=\"font-weight: 400;color: #333333\"><i>\u201cGa<em>s and dust from extremely metal-poor AGB stars\u201d,<\/em><\/i>\u00a02021, A&amp;A<\/span><\/span><\/strong><\/span><span style=\"color: #333333\"><strong><span style=\"font-weight: 400\"><span style=\"font-weight: 400;color: #333333\">, 655, A6<\/span><\/span><\/strong><\/span><\/li>\n<li style=\"font-weight: 400;text-align: justify\"><b>Yan Z., Jerabkova T., Kroupa P.,<\/b> <i><span style=\"font-weight: 400\">\u201cDownsizing revised: Star formation timescales for elliptical galaxies with an environment-dependent IMF and number of SNIa<\/span><\/i><span style=\"color: #333333\"><strong><span style=\"font-weight: 400\"><span style=\"font-weight: 400;color: #333333\"><i><em>\u201d,<\/em><\/i>\u00a02021, A&amp;A<\/span><\/span><\/strong><\/span><span style=\"color: #333333\"><strong><span style=\"font-weight: 400\"><span style=\"font-weight: 400;color: #333333\">, 655, A19<\/span><\/span><\/strong><\/span><\/li>\n<li><strong>Romano D.,<\/strong>\u00a0<i><span style=\"font-weight: 400\">\u201cThe evolution of CNO elements in galaxies<\/span><\/i><span style=\"color: #333333\"><strong><span style=\"font-weight: 400\"><span style=\"font-weight: 400;color: #333333\"><i><em>\u201d,<\/em><\/i> 2022, A&amp;ARv, 30, 7<\/span><\/span><\/strong><\/span><\/li>\n<\/ul>\n","protected":false},"excerpt":{"rendered":"<p>The discussions held in ISSI and ISSI-BJ and the support from ISSI\/ISSI-BJ are acknowledged in the following refereed publications: Kroupa P., Jerabkova T., \u201cThe Salpeter IMF and its descendants\u201d, 2019, Nat. Astr., 3, 482 Yan Z., Jerabkova T., Kroupa P., &hellip; <a href=\"https:\/\/www.issibern.ch\/teams\/chemabundism\/publications\/\">Continue reading <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-127","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.issibern.ch\/teams\/chemabundism\/wp-json\/wp\/v2\/pages\/127","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.issibern.ch\/teams\/chemabundism\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.issibern.ch\/teams\/chemabundism\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/chemabundism\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/chemabundism\/wp-json\/wp\/v2\/comments?post=127"}],"version-history":[{"count":0,"href":"https:\/\/www.issibern.ch\/teams\/chemabundism\/wp-json\/wp\/v2\/pages\/127\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.issibern.ch\/teams\/chemabundism\/wp-json\/wp\/v2\/media?parent=127"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}