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- W2029795110 abstract "view Abstract Citations (54) References (12) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Calculated Gamma-Ray Line Fluxes from the Type II Supernova 1987A Chan, L. W. ; Lingenfelter, R. E. Abstract Calculations of the time-dependent flux in the 847-keV gamma-ray line from the decay of Co-56 that might be expected from the type II supernova 1987 A in the LMC are presented. It is found that, for a wide range of assumed Co-56 and supernova ejecta masses, this line should be detectable by planned gamma-ray observations with flux sensitivities of about 0.0001 photons/sq cm sec. If this line is detected, the measurement of its time-dependent flux together with its width will make it possible to determine not only the mass of Co-56 produced by explosive nucleosynthesis, but also the total mass and energy of the ejecta, and hence the mass of the supernova's progenitor. Publication: The Astrophysical Journal Pub Date: July 1987 DOI: 10.1086/184936 Bibcode: 1987ApJ...318L..51C Keywords: Gamma Ray Spectra; Stellar Mass Ejection; Supernova 1987a; Cobalt Isotopes; Nuclear Fusion; Stellar Composition; Stellar Mass; Astrophysics; GAMMA RAYS: GENERAL; NUCLEOSYNTHESIS; STARS: SUPERNOVAE full text sources ADS | data products NED (2) SIMBAD (1)" @default.
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- W2029795110 date "1987-07-01" @default.
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- W2029795110 title "Calculated gamma-ray line fluxes from the Type II supernova 1987 A" @default.
- W2029795110 doi "https://doi.org/10.1086/184936" @default.
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