3D nebular spectra calculations for double-detonation Type Ia supernova models reveal viewing-angle dependent line profiles and tentatively support primary-only detonation over secondary detonation based on comparisons to observations.
@doi [ ] 10.1051/0004-6361:20030357, https://ui.adsabs.harvard.edu/abs/2003A&A...403..261L 403
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EP93 expansion opacities underestimate emissivity in radiative transfer; a modified bin-averaged method with expansion-adjusted line strength is proposed along with new public tables.
citing papers explorer
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Multidimensional Nebular-Phase Calculations of Dynamically-Driven Double-Degenerate Double-Detonation Models for Type Ia Supernovae
3D nebular spectra calculations for double-detonation Type Ia supernova models reveal viewing-angle dependent line profiles and tentatively support primary-only detonation over secondary detonation based on comparisons to observations.
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On Atomic Line Opacities for Modeling Astrophysical Radiative Transfer
EP93 expansion opacities underestimate emissivity in radiative transfer; a modified bin-averaged method with expansion-adjusted line strength is proposed along with new public tables.