Using late-time optical and near-infrared spectra to constrain Type Ia 
supernova explosion properties

Maguire, K.; Sim, S. A.; Shingles, L.; Spyromilio, J.; Jerkstrand, A.; Sullivan, M.; Chen, T.-W.; Cartier, R.; Dimitriadis, G.; Frohmaier, C.; Galbany, L.; Gutiérrez, C. P.; Hosseinzadeh, G.; Howell, D. A.; Inserra, C.; Rudy, R.; Sollerman, J.

doi:10.1093/mnras/sty820

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Using late-time optical and near-infrared spectra to constrain Type Ia supernova explosion properties

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Jerkstrand, A.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Chen, T.-W.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Maguire, K., Sim, S. A., Shingles, L., Spyromilio, J., Jerkstrand, A., Sullivan, M., et al. (2018). Using late-time optical and near-infrared spectra to constrain Type Ia supernova explosion properties. Monthly Notices of the Royal Astronomical Society, 477(3), 3567-3582. doi:10.1093/mnras/sty820.

Cite as: https://hdl.handle.net/21.11116/0000-0001-AA23-8

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