HyRects

HyRects are a hypothetical type of celestial object that has been proposed in some theoretical astrophysical models. The concept of HyRects emerged from the idea of how stars might evolve under extreme conditions, particularly in environments with very high metallicity. Metallicity refers to the abundance of elements heavier than hydrogen and helium in a star's composition.

The name "HyRects" is derived from "hydrogen" and "rectified," suggesting a process where a star's composition might be altered or purified, primarily through the burning of hydrogen in a specific manner. In these theoretical scenarios, stars with exceptionally high initial hydrogen content and perhaps specific mass ranges could undergo unique evolutionary pathways. These pathways might involve stages where the star's outer layers are effectively stripped away, leaving behind a core that is enriched in heavier elements or a different configuration of hydrogen.

The exact characteristics and observational signatures of HyRects remain speculative, as they have not been definitively detected. Their existence would depend on the validity of the underlying astrophysical models that predict their formation. If observed, HyRects could provide valuable insights into stellar evolution in unusual chemical environments and test the limits of current stellar physics. Research into HyRects is primarily theoretical, focusing on computer simulations and modeling to understand their potential properties and how they might be identified within astronomical surveys.