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The Nova Rate in NGC 2403

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arxiv 1210.0604 v2 pith:CA5R6376 submitted 2012-10-02 astro-ph.SR

J. R. Franck , A. W. Shafter , K. Hornoch , K. A. Misselt This is my paper · ORCID
classification astro-ph.SR
keywords novarateyeargalaxyluminositiesnovaesolarapril
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A multi-epoch H-alpha survey of the late-type spiral galaxy NGC 2403 has been completed in order to determine its nova rate. A total of 9 nova candidates were discovered in 48 nights of observation with two different telescopes over the period from February 2001 to April 2012. After making corrections for temporal coverage and spatial completeness, a nova rate of 2.0 (+0.5,-0.3) per year was determined. This rate corresponds to a luminosity-specific nova rate of 2.5+/-0.7 novae per year per 10^{10} solar luminosities in K. This value is consistent with that of the similar Hubble type galaxy, M33, and is typical of those of other galaxies with measured nova rates, which range from 1-3 novae per year per 10^{10} solar luminosities in K.

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  1. Association between Recurrent Novae and Nova Super-Remnants

    astro-ph.GA 2024-11 conditional novelty 2.0 of 10

    A review of nova super-remnants: the prototypical M31N 2008-12a remnant, new Galactic examples around KT Eridani and RS Ophiuchi, and a survey finding none in M31 or the LMC.

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