Not exact matches
H1504 +65 is the hottest
white dwarf on record — and the only known
star lacking
helium and hydrogen.
«It tells us that nature has found a way that we didn't know to make
white dwarf stars without the usual hydrogen or
helium surface layers,» Dufour says.
The first so - called
helium nova, the possible result of a large
white dwarf sucking material from a hydrogen - deficient companion
star, may be a precursor to a supernova
Radiation from the
white dwarf star, the
white dot in the center of the ring, is exciting the
helium to glow.
«The formation of such a binary system containing an extremely low mass
helium white dwarf has to be the result of interactions and mass loss between the two original
stars,» said Howell.
Astrophysicists at UC Santa Barbara are the first scientists to identify two
white dwarf stars in an eclipsing binary system, allowing for the first direct radius measurement of a rare
white dwarf composed of pure
helium.
As US 708 traveled around the
white dwarf, the dead
star would have stolen its
helium.
One of the
stars in the newly discovered binary is a relatively rare
helium - core
white dwarf with a mass only 10 to 20 percent of that of the sun.