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  • Current Galactic Chemical Evolution models fail to explain rising Na-abundances of young thick disc stars
    • Volume 20, Issue 18 - article #2
    • E. K. Owusu (School of Science, University of New South Wales Canberra, Australia Defence Force Academy, Australia, ARC Centre of Excellence for All-Sky Astrophysics in 3 Dimensions, Max-Planck-Institut f"ur Astronomie, Heidelberg, Germany, Heidelberger Institut f"ur Theoretische Studien, Heidelberg, Germany), A. J. Ruiter (School of Science, University of New South Wales Canberra, Australia Defence Force Academy, Australia, ARC Centre of Excellence for All-Sky Astrophysics in 3 Dimensions, Max-Planck-Institut f"ur Astronomie, Heidelberg, Germany, Heidelberger Institut f"ur Theoretische Studien, Heidelberg, Germany, OzGrav: The ARC Centre of Excellence for Gravitational Wave Discovery, Hawthorn, Australia), A. J. Kemp (Institute of Astronomy), S. Buder (ARC Centre of Excellence for All-Sky Astrophysics in 3 Dimensions, Research School of Astronomy, Astrophysics, Australian National University, Australia), I. R. Seitenzahl (Heidelberger Institut f"ur Theoretische Studien, Heidelberg, Germany), N. Rodriguez-Segovia (School of Science, University of New South Wales Canberra, Australia Defence Force Academy, Australia), R. Pakmor (Max Planck Institute for Astrophysics, Garching, Germany), G. C. Cinquegrana (ARC Centre of Excellence for All-Sky Astrophysics in 3 Dimensions, School of Physics, Astronomy, Monash University, Clayton, Australia), N. Storm (Max-Planck-Institut f"ur Astronomie, Heidelberg, Germany, Heidelberg University, Heidelberg, Germany), P. Eitner (Max-Planck-Institut f"ur Astronomie, Heidelberg, Germany, Heidelberg University, Heidelberg, Germany), M. Bergemann (Max-Planck-Institut f"ur Astronomie, Heidelberg, Germany)
    • https://arxiv.org/abs/2506.17711
  • APOKASC-3: The Third Joint Spectroscopic and Asteroseismic catalog for Evolved Stars in the Kepler Fields
    • Volume 19, Issue 40 - article #1
    • Marc H. Pinsonneault (Department of Astronomy, The Ohio State University, USA), Joel C. Zinn (Department of Physics, California State Long Beach, USA), Jamie Tayar (Department of Astronomy, University of Florida, USA), Aldo Serenelli (Institute of Space Sciences, ICE, CSIC, Spain, Institut d'Estudis Espacials de Catalunya, Spain), Rafael A. Garcia (Universite Paris Cite, CEA, CNRS, France), Savita Mathur (Instituto de Astrofsica de Canarias, Spain, Departamento de Astrofisica Universidad de La Laguna, Spain, Space Science Institute, USA), Mathieu Vrard (Department of Astronomy, The Ohio State University, USA, Observatoire de la Cote d'Azur CNRS, France), Yvonne P. Elsworth (School of Physics, Astronomy, University of Birmingham, UK, Stellar Astrophysics Centre, Department of Physics, Astronomy, Aarhus University, Denmark), Benoit Mosser (LESIA Observatoire de Paris Universite, PSL, CNRS, Sorbonne Universite, Universite de Paris, France), Dennis Stello (School of Physics, University of New South Wales, Australia, Sydney Institute for Astronomy, School of Physics, University of Sydney, Australia, ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions, Australia), Keaton J. Bell (Department of Physics, Queens College, CUNY, USA), Lisa Bugnet (Institute of Science, Technology Austria), Enrico Corsaro (INAF, Osservatorio Astrofisico di Catania, Italy), Patrick Gaulme (Thuringer Landessternwarte, Germany, Department of Astronomy, New Mexico State University, USA), Saskia Hekker (Stellar Astrophysics Centre, Department of Physics, Astronomy, Aarhus University, Denmark, Heidelberg University, Germany, Heidelberg Institute for Theoretical Studies, Germany), Marc Hon (Kavli Institute for Astrophysics, Space Research, Massachusetts Institute of Technology, USA, Institute for Astronomy, University of Hawaii, USA), Daniel Huber (Institute for Astronomy, University of Hawaii, USA, SIfA, School of Physics, University of Sydney, Australia), Thomas Kallinger (Institute for Astronomy, University of Vienna, Austria), Kaili Cao (Center for Cosmology, AstroParticle Physics, Department of Physics, The Ohio State University, USA), Jennifer A. Johnson (Department of Astronomy, The Ohio State University, USA, Center for Cosmology, AstroParticle Physics), Bastien Liagre (Universite Paris Cite, CEA, CNRS, France, Instituto de Astrofsica de Canarias, Spain, ENS Paris-Saclay, Universite Paris-Saclay, France), Rachel A. Patton (Department of Astronomy, The Ohio State University, USA, Center for Cosmology, AstroParticle Physics), Angela R. G. Santos (Instituto de Astrofisica e Ciencias do Espac{c}o, Universidade do Porto, Portugal), Sarbani Basu (Department of Astronomy, Yale University, USA), Paul G. Beck (Instituto de Astrofsica de Canarias, Spain, Departamento de Astrofisica Universidad de La Laguna, Spain), Timothy C. Beers (Dept. of Physics, Astronomy,, JINA Center for the Evolution of the Elements University of Notre Dame, USA), William J. Chaplin (School of Physics, Astronomy, University of Birmingham, UK, Stellar Astrophysics Centre, Department of Physics, Astronomy, Aarhus University, Denmark), Katia Cunha (University of Arizona, Steward Observatory, USA, Observatorio Nacional, Sao Cristovao, Brazil), Peter M. Frinchaboy (Department of Physics, Astronomy, Texas Christian University, USA, Maunakea Spectroscopic Explorer, Canada-France-Hawaii-Telescope, USA), Leo Girardi (Osservatorio Astronomico di Padova, INAF, Italy), Diego Godoy-Rivera (Instituto de Astrofsica de Canarias, Spain, Departamento de Astrofisica Universidad de La Laguna, Spain), Jon A. Holtzman (Department of Astronomy, New Mexico State University, USA), Henrik Jonsson (Materials Science, Applied Mathematics, Malmo University, Sweden), Szabolcs Meszaros (ELTE Eotvos Lorand University, Gothard Astrophysical Observatory, Hungary, MTA-ELTE Lendulet Momentum Milky Way Research Group, Hungary), Claudia Reyes (School of Physics, University of New South Wales, Australia), Hans-Walter Rix (Max Planck Institute for Astronomy, Heidelberg, Germany), Matthew Shetrone (University of California Observatories, University of California Santa Cruz, USA), Verne V. Smith (NSFs NOIRLab, USA), Taylor Spoo (Department of Physics, Astronomy, Texas Christian University, USA), Keivan G. Stassun (Department of Physics, Astronomy, Vanderbilt University, USA), Ji Wang (Department of Astronomy, The Ohio State University, USA)
    • https://arxiv.org/abs/2410.00102
  • Constraining Nucleosynthesis in Two CEMP Progenitors Using Fluorine. (arXiv:2008.10136v1 [astro-ph.SR])
    • Volume 15, Issue 35 - article #2
    • A. A. Mura-Guzmán (1,2), D. Yong (1,2), C. Abate (3), A. Karakas (4,2), C. Kobayashi (5,2), H. Oh (6), S. Chun (6), G. Mace (7). ((1) Research School of Astronomy, Astrophysics, Australian National University, Australia, (2) ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia, (3) Deep Blue Srl, Rome, Italy, (4) School of Physics, Astronomy, Monash University, Australia, (5) Centre for Astrophysics Research, University of Hertfordshire, UK, (6) Korea Astronomy, Space Science Institute, Republic of Korea, (7) Department of Astronomy, McDonald Observatory, University of Texas at Austin, USA.)
    • http://arxiv.org/abs/2008.10136
  • Building galaxies by accretion and in situ star formation
  • A New Approach to the Solar Oxygen Abundance Problem
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