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Иш: A Comparison of Three Neodymium Atomic Data Sets for Kilonova Modeling
[CLC][ITAL]r[/ITAL][/CLC]-Process in Neutron Star Mergers
C. Freiburghaus, Stephan Rosswog, F.‐K. Thielemann
Мақола19996 иқтибосABIA kilonova as the electromagnetic counterpart to a gravitational-wave source
Stephen Smartt, T. W. Chen, Anders Jerkstrand +97
Мақола20175 иқтибосABIOn the astrophysical robustness of the neutron star merger r-process
O. Korobkin, S. Rosswog, A. Arcones +1
Мақола20125 иқтибосABISystematic opacity calculations for kilonovae
Masaomi Tanaka, Daiji Kato, Gediminas Gaigalas +1
Мақола20204 иқтибосABINLTE effects on kilonova expansion opacities
Quentin Pognan, Anders Jerkstrand, Jon Grumer
Мақола20224 иқтибосABIThe X-ray counterpart to the gravitational-wave event GW170817
E. Troja, L. Piro, Hendrik van Eerten +31
Мақола20173 иқтибосABIIdentification of strontium in the merger of two neutron stars
D. Watson, C. J. Hansen, J. Selsing +15
Мақола20193 иқтибосABINebular Emission from Lanthanide-rich Ejecta of Neutron Star Merger
Kenta Hotokezaka, Masaomi Tanaka, Daiji Kato +1
Мақола20213 иқтибосABIOn the validity of steady-state for nebular phase kilonovae
Quentin Pognan, Anders Jerkstrand, Jon Grumer
Мақола20213 иқтибосABI