r-Process elements from magnetorotational hypernovae
David YongARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Canberra, Australian Capital Territory, Australia. [email protected]Chiaki KobayashiARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Canberra, Australian Capital Territory, AustraliaG. S. Da CostaARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Canberra, Australian Capital Territory, AustraliaM. S. BessellResearch School of Astronomy and Astrophysics, Australian National University, Canberra, Australian Capital Territory, AustraliaAnirudh ChitiDepartment of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USAAnna FrebelDepartment of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USAK. LindDepartment of Astronomy, Stockholm University, AlbaNova University Center, Stockholm, SwedenDougal MackeyARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Canberra, Australian Capital Territory, AustraliaThomas NordlanderARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Canberra, Australian Capital Territory, AustraliaM. AsplundMax Planck Institute for Astrophysics, Garching, GermanyAndrew R. CaseyARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Canberra, Australian Capital Territory, AustraliaA. F. MarinoIstituto Nazionale di Astrofisica - Osservatorio Astronomico di Arcetri, Florence, ItalySimon J. MurphyResearch School of Astronomy and Astrophysics, Australian National University, Canberra, Australian Capital Territory, AustraliaB. SchmidtResearch School of Astronomy and Astrophysics, Australian National University, Canberra, Australian Capital Territory, Australia
2021en
ABI
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