{"id":27,"date":"2015-06-30T22:18:23","date_gmt":"2015-06-30T20:18:23","guid":{"rendered":"http:\/\/www.issibern.ch\/teams\/labtostars\/?page_id=27"},"modified":"2015-06-30T22:18:23","modified_gmt":"2015-06-30T20:18:23","slug":"publications","status":"publish","type":"page","link":"https:\/\/www.issibern.ch\/teams\/labtostars\/publications\/","title":{"rendered":"Publications"},"content":{"rendered":"<ul>\n<li>Thermonuclear Bursts with Short Recurrence Times from Neutron Stars Explained by Opacity-Driven Convection. 2017, <a href=\"http:\/\/adsabs.harvard.edu\/abs\/2017ApJ...842..113K\">ApJ 842(2), #113<\/a>,\u00a0Keek, L. &amp; Heger, A<\/li>\n<li>Dependence of X-ray Burst Models on Nuclear Masses, 2017, accepted by\u00a0ApJ (<a href=\"https:\/\/arxiv.org\/abs\/1610.07596\">arXiv:1610.07596<\/a>), Hendrik Schatz &amp; Wei-Jia Ong<\/li>\n<li>Flux decay during thermonuclear X-ray bursts analysed with the dynamic power-law index method, 2017, accepted by A&amp;A \u00a0(<a href=\"https:\/\/arxiv.org\/abs\/1705.05653\">arXiv:1705.05653<\/a>)\u00a0Kuuttila, J.; Kajava, J. J. E.; N\u00e4ttil\u00e4, J.; Motta, S. E.; S\u00e1nchez-Fern\u00e1ndez, C.; Kuulkers, E.; Cumming, A.; Poutanen, J.<\/li>\n<li>IGR J17062\u20136143 Is an Accreting Millisecond X-Ray Pulsar,\u00a02017,\u00a0<a href=\"http:\/\/adsabs.harvard.edu\/abs\/2017ApJ...836L..23S\">ApJ Lett. 836, L23<\/a>,\u00a0Strohmayer, Tod &amp; Keek, Laurens<\/li>\n<li>X-Ray Reflection and an Exceptionally Long Thermonuclear Helium Burst from IGR J17062-6143,\u00a02017, <a href=\"http:\/\/adsabs.harvard.edu\/abs\/2017ApJ...836..111K\">ApJ 836, #111<\/a>,\u00a0Keek, L., Iwakiri, W., Serino, M., Ballantyne, D. R., in\u2019t Zand, J. J. M., &amp; Strohmayer, T. E.<\/li>\n<li>Thermonuclear Burst Observations for Model Comparisons: A Reference Sample, 2017, <a href=\"https:\/\/www.cambridge.org\/core\/journals\/publications-of-the-astronomical-society-of-australia\/article\/thermonuclear-burst-observations-for-model-comparisons-a-reference-sample\/8945B2BBD6094AED3D700D377210BCF4\">PASA 34, e019<\/a>\u00a0(e-print at <a href=\"https:\/\/arxiv.org\/abs\/1703.07485\">arXiv:1703.07485<\/a>, on-line data also at <a href=\"http:\/\/burst.sci.monash.edu\/reference\">http:\/\/burst.sci.monash.edu\/reference<\/a>) Duncan Galloway, Adelle Goodwin, &amp; Laurens Keek<\/li>\n<li>Constraints on Bygone Nucleosynthesis from Accreting Neutron Stars, 2017, <a href=\"http:\/\/adsabs.harvard.edu\/abs\/2017ApJ...837...73M\">ApJ 837, #73<\/a> (<a href=\"https:\/\/arxiv.org\/abs\/1701.02730\">arXiv:1701.02730<\/a>), Zach Meisel &amp; Alex Deibel<\/li>\n<li>Detection of burning ashes from thermonuclear X-ray bursts, 2017,\u00a0<a href=\"http:\/\/adsabs.harvard.edu\/abs\/2017MNRAS.464L...6K\">MNRAS 464, L6-10<\/a>,\u00a0Kajava, J. J. E.; N\u00e4ttil\u00e4, J.; Poutanen, J.; Cumming, A.; Suleimanov, V.; Kuulkers, E.<\/li>\n<li>A Survey of Chemical Separation in Accreting Neutron Stars, 2016, <a href=\"http:\/\/adsabs.harvard.edu\/abs\/2016ApJ...823..117M\">ApJ 823, #117<\/a>,\u00a0Mckinven, Ryan; Cumming, Andrew; Medin, Zach; Schatz, Hendrik<\/li>\n<li>Accretion Disk Signatures in Type I X-Ray Bursts: Prospects for Future Missions, 2016, <a href=\"http:\/\/adsabs.harvard.edu\/abs\/2016ApJ...826...79K\">ApJ 826, #79<\/a>,\u00a0Keek, L., Wolf, Z., &amp; Ballantyne, D. R. 2016<\/li>\n<li>Anisotropy of X-Ray Bursts from Neutron Stars with Concave Accretion Disks, 2016, <a href=\"http:\/\/adsabs.harvard.edu\/abs\/2016ApJ...819...47H\">ApJ 819, #47<\/a>,\u00a0He, C.-C. &amp; Keek, L.<\/li>\n<li>Urca cooling pairs in the neutron star ocean and their effect on superbursts, 2016, <a href=\"http:\/\/adsabs.harvard.edu\/abs\/2016ApJ...831...13D\">ApJ 831, #13<\/a> (<a href=\"http:\/\/adsabs.harvard.edu\/abs\/2016arXiv160301281D\">arXiv:160301281<\/a>), Alex Deibel, Zach Meisel, Hendrik Schatz, Ed Brown, and Andrew Cumming.<\/li>\n<\/ul>\n","protected":false},"excerpt":{"rendered":"<p>Thermonuclear Bursts with Short Recurrence Times from Neutron Stars Explained by Opacity-Driven Convection. 2017, ApJ 842(2), #113,\u00a0Keek, L. &amp; Heger, A Dependence of X-ray Burst Models on Nuclear Masses, 2017, accepted by\u00a0ApJ (arXiv:1610.07596), Hendrik Schatz &amp; Wei-Jia Ong Flux decay &hellip; <a href=\"https:\/\/www.issibern.ch\/teams\/labtostars\/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-27","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.issibern.ch\/teams\/labtostars\/wp-json\/wp\/v2\/pages\/27","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.issibern.ch\/teams\/labtostars\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.issibern.ch\/teams\/labtostars\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/labtostars\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/labtostars\/wp-json\/wp\/v2\/comments?post=27"}],"version-history":[{"count":0,"href":"https:\/\/www.issibern.ch\/teams\/labtostars\/wp-json\/wp\/v2\/pages\/27\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.issibern.ch\/teams\/labtostars\/wp-json\/wp\/v2\/media?parent=27"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}