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Systematically Bridging the Gap between Novae and Supernovae

Published online by Cambridge University Press:  17 January 2013

Mansi M. Kasliwal
Mansi M. Kasliwal*
Affiliation:
Department of Astronomy, California Institute of Technology, 1200 E. California Blvd. M/C 249-17, Pasadena CA 91125, USA Carnegie Institution for Science, 813 Santa Barbara St, Pasadena, CA 91101, USA Hubble Fellow and Carnegie-Princeton Fellow email: mansi@obs.carnegiescience.edu
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Abstract

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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.

Keywords

surveys — stars: novaecataclysmic variablessupernovae
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Issue S281: Binary Paths to Type Ia Supernovae Explosions , July 2011 , pp. 9 - 16
Copyright
Copyright © International Astronomical Union 2013

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