"I thought I had found a pair in 1936 (V630 Sgr and V368 Aql)," he says. "But I looked at their light curves, and it turns out they were not at maximum brightness at the same time."
These appear to be classical novas. First documented by Chinese astronomers some 2000 years ago, the explosions occur in binary star systems. White dwarf stars steal gas from a bloated partner until the stolen fuel ignites in a sudden thermonuclear blast. It's less dramatic than a supernova, but still an awesome blast.
Nova V462 Lupi is currently near magnitude +5.9, while V572 Velorum, fading from a peak near +4.8, is the brighter of the two. Southern astronomers, this may not happen again for a loooong time.
https://spaceweather.com/