Systematically bridging the gap between novae and supernovae

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Abstract

The venerable study of cosmic explosions is over a century old. However, until recently, there has existed a glaring six-magnitude luminosity gap between the brightest novae and faintest supernovae. To find optical transients that are fainter, faster, and rarer than supernovae, we designed a systematic search: the Palomar Transient Factory. Theorists predict a variety of mechanisms to produce transients in the gap and observers have the best chance of finding them in the local universe. Here I present discoveries and unique physics of cosmic explosions that bridge this gap between novae and supernovae. Copyright © International Astronomical Union 2013.

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APA

Kasliwal, M. M. (2013). Systematically bridging the gap between novae and supernovae. In Proceedings of the International Astronomical Union (Vol. 7, pp. 9–16). Cambridge University Press. https://doi.org/10.1017/S1743921312014585

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