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From supernova to supernova remnant: comparison of thermonuclear explosion models
Gilles Ferrand, Donald C. Warren, Masaomi Ono +6
Progress in the three-dimensional modeling of supernovae (SN) prompts us to revisit the supernova remnant (SNR) phase. We continue our study of the imprint of a thermonuclear explo…
LIN 358: A symbiotic binary accreting above the steady hydrogen fusion limit
J. Kuuttila, M. Gilfanov, T. E. Woods +2
Symbiotic binaries are long period interacting binaries consisting of a white dwarf (WD) accreting material from a cool evolved giant star via stellar winds. In this paper we study…
A supernova remnant associated with a nascent black hole low-mass X-ray binary
N. I. Maxted, A. J. Ruiter, K. Belczynski +2
Energy released when the core of a high-mass star collapses into a black hole often powers an explosion that creates a supernova remnant. Black holes have limited windows of observ…
New Optically Identified Supernova Remnants in the Large Magellanic Cloud
Miranda Yew, Miroslav D. Filipović, Milorad Stupar +20
We present a new optical sample of three Supernova Remnants and 16 Supernova Remnant (SNR) candidates in the Large Magellanic Cloud(LMC). These objects were originally selected usi…
Nucleosynthesis imprints from different Type Ia Supernova explosion scenarios and implications for galactic chemical evolution
F. Lach, F. K. Roepke, I. R. Seitenzahl +3
We analyze the nucleosynthesis yields of various Type Ia supernova explosion simulations including pure detonations in sub- Chandrasekhar mass white dwarfs, double detonations and…
Imagery and UV Spectroscopy of the LMC Supernova Remnant N103B Using HST
William P. Blair, Parviz Ghavamian, John C. Raymond +6
We present HST/WFC3 multiband imagery of N103B, the remnant of a Type Ia supernova in the Large Magellanic Cloud, as well as HST/COS ultraviolet spectroscopy of the brightest radia…