A Mystery in Chamaeleon: Serendipitous Discovery of a Galactic Symbiotic Nova
arXiv:2002.07852 · doi:10.3847/1538-3881/aba435
Abstract
We present the serendipitous discovery of a low luminosity nova occurring in a symbiotic binary star system in the Milky Way. We lay out the extensive archival data alongside new follow-up observations related to the stellar object V CN Cha in the constellation of Chamaeleon. The object had long period (day), high amplitude (mag) optical variability in its recent past, preceding an increase in optical brightness by magnitudes and a persistence at this luminosity for about 3 years, followed by a period of dimming. The object's current optical luminosity seems to be dominated by H emission, which also exhibits blue-shifted absorption (a P-Cygni-like profile). After consideration of a number of theories to explain these myriad observations, we determine that V CN Cha is most likely a symbiotic (an evolved star-white dwarf binary) system which has undergone a long-duration, low luminosity, nova. Interpreted in this way, the outburst in V CN Cha is among the lowest luminosity novae ever observed.
Submitted to AJ, 19 pages, 9 figure
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