PoS - Proceedings of Science
Volume 255 - The Golden Age of Cataclysmic Variables and Related Objects - III (Golden2015) - Classical Novae, Recurrent Novae and Nova-Like Stars
Classical novae in OGLE data
P. Mroz* and  On behalf of OGLE collaboration
Full text: pdf
Pre-published on: February 10, 2017
Published on: May 23, 2017
Abstract
I present the results of a systematic search for classical novae in the Galactic bulge and Magellanic Clouds in data from the OGLE survey. I measured nova rates in all those environments: 13.8 +/- 2.6 per yr(Milky Way bulge), 2.4 +/- 0.8 per yr (LMC), and 0.9 +/- 0.4 per yr (SMC). The K-band luminosity-specific nova rate in the Galactic bulge is significantly higher than in other galaxies, suggesting different nova rates per unit mass in different Galactic populations. I also provide strong upper limits on the number of very frequently erupting recurrent novae, which indicates they cannot be a significant channel of SN Ia progenitors. Finally, I identified several post-nova candidates based on their photometric variability.
DOI: https://doi.org/10.22323/1.255.0054
How to cite

Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in "proceeding" format which is more detailed and complete.

Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.