[Tee tiong huat]

All 3-options remain on table, way to figure out will to examine chemical composition of star in greater detail. If J1249+36 was companion of a white dwarf, the supernova could have left trace elements that polluted the subdwarf's atmosphere. Conversely, globular clusters contain stars that all have similar compositional properties, so it may be possible to link population that way.

If neither of those pan out, we may need to look to Milky Way's satellites, to determine whether tiny, dim star is a stranger from outside galaxy, just winking howdy as it passes through us. This discovery was presented at 224th meeting of American Astronomical Society.

This tiny, so tiny so small things go on with their live, a life of their own. They don't need Oxygen (Ox) to live (in Life) in Venes.

https://youtube.com/shorts/vieaHzbfeGg?s...KwmN28rjb1