Hydrodynamic simulations of white dwarf-white dwarf mergers and the origin of R Coronae Borealis stars
Artikel i vetenskaplig tidskrift, 2024
stars: evolution
hydrodynamics
white dwarfs
binaries: close
stars: carbon
methods: numerical
Författare
Sagiv Shiber
Louisiana State University
Orsola De Marco
Macquarie University
Patrick M. Motl
Indiana Univ Kokomo, Sch Sci
Bradley Munson
McMaster University
Louisiana State University
Dominic C. Marcello
Louisiana State University
Louisiana State Univ, LSU Ctr Computat & Technol
Juhan Frank
Louisiana State University
Patrick Diehl
Louisiana State Univ, LSU Ctr Computat & Technol
Los Alamos Natl Lab, Appl Comp Sci CCS 7
Louisiana State University
Geoffrey C. Clayton
Louisiana State University
Bennett N. Skinner
McMaster University
University of Arizona
Hartmut Kaiser
Louisiana State Univ, LSU Ctr Computat & Technol
Louisiana State Univ, Div Comp Sci & Engn
Gregor Daiss
Louisiana State Univ, LSU Ctr Computat & Technol
Universität Stuttgart
Dirk Pflueger
Universität Stuttgart
Jan Staff
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Monthly Notices of the Royal Astronomical Society
0035-8711 (ISSN) 1365-2966 (eISSN)
Vol. 535 2 1914-1943Ämneskategorier
Astronomi, astrofysik och kosmologi
DOI
10.1093/mnras/stae2343