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Title:
Systematically Bridging the Gap between Novae and Supernovae
Authors:
Kasliwal, Mansi M.
Affiliation:
AA(Department of Astronomy, California Institute of Technology, 1200 E. California Blvd. M/C 249-17, Pasadena CA 91125, USA)
Publication:
Binary Paths to Type Ia Supernovae Explosions, Proceedings of the International Astronomical Union, IAU Symposium, Volume 281, p. 9-16
Publication Date:
01/2013
Origin:
CUP
Keywords:
surveys, stars: novae, cataclysmic variables, supernovae,
Abstract Copyright:
(c) 2013: Copyright © International Astronomical Union 2013
DOI:
10.1017/S1743921312014585
Bibliographic Code:
2013IAUS..281....9K

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.

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