Gaia sees strange stars in most detailed Milky Way survey to date
esa.int
esa.int
What does the current theory say and how big of a development is this observation?
Relatedly, given how far we’re starting to push the tech with our observation tools, how certain are we that our observations aren’t synthetic artifacts of the algorithms used to process sensors and generate the results? I’m guessing there’s cross-correlation done with existing observations on other HW/SW that’s used to reduce the probability of that kind of issue. Wonder though if there’s some kind of SW development techniques they employ that could be useful elsewhere in the industry.
My prediction would be heavier elements increase in occurrence in near the center of the galaxy. But, huge grain of salt.
> Stars that are closer to the centre and plane of our galaxy are richer in metals than stars at larger distances.