OGLE Atlas of Classical Novae I. Galactic Bulge Objects

TL;DR

This paper presents a precise measurement of the Galactic bulge nova rate using OGLE data, analyzes nova light curves, and estimates orbital periods, providing new insights into nova populations and recurrence in the bulge.

Contribution

The study provides the first accurate nova rate for the Galactic bulge and detailed analysis of nova light curves and orbital periods based on long-term OGLE observations.

Findings

Galactic bulge nova rate is 13.8 ± 2.6 per year.

No recurrent novae similar to M31 2008-12a detected.

Orbital periods were measured for 18 post-novae and novae.

Abstract

Eruptions of classical novae are possible sources of lithium formation and gamma-ray emission. Nova remnants can also become Type Ia supernovae (SNe Ia). The contribution of novae to these phenomena depends on nova rates, which are not well established for the Galaxy. Here, we directly measure a Galactic bulge nova rate of $13.8 \pm 2.6$ per year. This measurement is much more accurate than any previous measurement of this kind thanks to many years' monitoring of the bulge by the Optical Gravitational Lensing Experiment (OGLE) survey. Our sample consists of 39 novae eruptions, $\sim$1/3 of which are OGLE-based discoveries. This long-term monitoring allows us to not only measure the nova rate but also to study in detail the light curves of 39 eruptions and more than 80 post-nova candidates. We measured orbital periods for 9 post-novae and 9 novae, and in 14 cases we procured the first estimates. The OGLE survey is very sensitive to the frequently erupting recurrent novae. We did not find any object similar to M31 2008-12a, which erupts once a year. The lack of detection indicates that there is only a small number of them in the Galactic bulge.