A ONe nova occurs when matter builds up on the surface of an oxygen-neon-magnesium rich white dwarf star and is heated to the point to ignite explosive run-away nuclear fusion.

During those very early moments of the universe, things were extraordinarily hot, and quark-gluon plasma behaves in strange ways when super-heated. This is because high temperatures will bring on ...

Oxygen-neon, or oxygen-neon-magnesium novae, also known as ONe novae, have been suspected since the late 1990s of forming phosphorus in abundance by a complex fusion path, ...

Experts shared their thoughts on the best high-frequency skincare wands for clearer, firmer skin. Here are their picks from ...

These elements include oxygen, iron, neon, magnesium, silicon, argon, calcium, nickel, and – detected for the first time ever in a galaxy cluster – chromium.

Once the Oxygen/Neon White Dwarf star approaches the Chandrasekhar limit for rotationally supported white dwarf stars, it undergoes accretion induced collapse to form a neutron star.

A ONe nova occurs when matter builds up on the surface of an oxygen-neon-magnesium rich white dwarf star and is heated to the point to ignite explosive run-away nuclear fusion.

New techniques and refinements of older ones are needed to reach <1 K for quantum-computing cooling. Part 1 provided an ...

Helium, oxygen, neon, iron—they all come from the fusion that takes place in dying stars. But we have a lot of elements that are more massive than iron; it’s only element 26 of 118, after all.