Supernova SN 2011fe from an exploding carbon-oxygen white dwarf star.

Supernova SN 2011fe from an exploding carbon-oxygen white dwarf star.

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Type Ia supernovae have been used empirically as 'standard candles' to demonstrate the acceleration of the expansion of the Universe even though fundamental details, such as the nature of their progenitor systems and how the stars explode, remain a mystery. There is consensus that a white...

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التفاصيل البيبلوغرافية
المؤلفون الرئيسيون: Nugent, P, Sullivan, M, Cenko, S, Thomas, R, Kasen, D, Howell, D, Bersier, D, Bloom, J, Kulkarni, SR, Kandrashoff, M, Filippenko, A, Silverman, J, Marcy, G, Howard, A, Isaacson, H, Maguire, K, Suzuki, N, Tarlton, J, Pan, Y, Bildsten, L, Fulton, B, Parrent, J, Sand, D, Podsiadlowski, P, Bianco, F
التنسيق: Journal article
اللغة:English
منشور في: 2011

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