| http://www.w3.org/ns/prov#value | - of radioactive isotopes suggests that this scenario may not be so likely.Whatever the cause, these new features are a reminder that there is much we still do not understand about our own local universe.Theoretical models of the evolution of massive stars suggest that, for stars over a certain mass limit, the likely end result is a black hole, the compressed remnant of a stellar core which is so mas
|
