In other cases, another member of the system will go on to form a second white dwarf. If gravitational instabilities bring ...

A semi-explicit time domain method for solving eddy current problems is presented. The suggested method is based on the discontinuous Galerkin (DG) finite-element approach and the H-Φ formulation of ...

The precursors of heavy elements might arise in the plasma underbellies of swollen stars or in smoldering stellar corpses. They definitely exist in East Lansing, Michigan.

An international team of researchers, led by scientists from GSI/FAIR in Darmstadt, Germany, has studied r-process ...