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How Far Can We Trust Type Ia Supernovae as Standard Candles?

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White Dwarfs: Cosmological and Galactic Probes

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 332))

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Abstract

We review the various possibilities that have been proposed as progenitors of Type Ia supernovae (SNe Ia) from the point of view of binary evolution and population synthesis. Depending on the nature of the progenitor, there may be systematic effects that cannot be calibrated by local observations that could undermine their use as standard candles.

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© 2005 Springer

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Wickramasinghe, D., Tout, C.A., Regős, E., Hurley, J., Pols, O. (2005). How Far Can We Trust Type Ia Supernovae as Standard Candles?. In: Sion, E.M., Vennes, S., Shipman, H.L. (eds) White Dwarfs: Cosmological and Galactic Probes. Astrophysics and Space Science Library, vol 332. Springer, Dordrecht. https://doi.org/10.1007/1-4020-3725-2_16

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