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On the AGB stars of M4: A robust disagreement between spectroscopic observations and theory

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Based in part on data acquired through the AAO, via programs 09B/15, 14B/27, and 15A/21 (PI: Campbell); some of these observations were conducted by Elizabeth Wylie de Boer, Richard Stancliffe,… Click to show full abstract

Based in part on data acquired through the AAO, via programs 09B/15, 14B/27, and 15A/21 (PI: Campbell); some of these observations were conducted by Elizabeth Wylie de Boer, Richard Stancliffe, and George Angelou. Part of this work was supported by the DAAD (PPP project 57219117) with funds from the German Federal Ministry of Education and Research (BMBF). Parts of this research were conducted by the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013. BTM acknowledges the financial support of the Research Training Program (RTP) scheme scholarship. SWC acknowledges federal funding from the Australian Research Council though the Future Fellowship grant entitled ‘Where are the Convective Boundaries in Stars?’ (FT160100046). AMA acknowledges funds from the Alexander von Humboldt Foundation in the framework of the Sofja Kovalevskaja Award endowed by the Federal Ministry of Education and Research. TN acknowledges funding from the Australian Research Council (grant DP150100250). VD acknowledges support from the AAO distinguished visitor programme 2016. LC gratefully acknowledges support from the Australian Research Council (grants DP150100250, FT160100402). This work was supported by computational resources provided by the Australian Government through the National Computational Infrastructure (NCI) under the National Computational Merit Allocation Scheme (project ew6).

Keywords: research council; research; agb stars; australian research; stars robust

Journal Title: Monthly Notices of the Royal Astronomical Society
Year Published: 2018

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