It may be the remains of a carbon -
rich white dwarf star.
Not exact matches
Creating so much oxygen takes a fiercer nuclear furnace than is needed for a carbon -
rich mixture, so the
stars that became these
white dwarfs must have been hot and massive.
WHAT LIES WITHIN The inner structure of a
white dwarf star (shown in this artist's impression) has been mapped for the first time — and it's more oxygen -
rich than expected.
There are many
white dwarfs that hold large amounts of hydrogen in their atmospheres, and this new study suggests that this is evidence that water -
rich asteroids or comets are common around other
stars than the Sun.»
Artist's impression of a rocky and water -
rich asteroid being torn apart by the strong gravity of the
white dwarf star.
Today, a UCLA - led team of scientists reports that it has discovered the existence of a
white dwarf star whose atmosphere is
rich in carbon and nitrogen, as well as in oxygen and hydrogen, the components of water.
Artist impression of a rocky and water -
rich asteroid being torn apart by the strong gravity of the
white dwarf star GD 61.
A UCLA - led team of scientists discovered a
white dwarf star in the constellation Boötes whose atmosphere is
rich in carbon, nitrogen, oxygen and hydrogen.
HD 147513 A is a so - called young «Barium
dwarf» (s - process element
rich but comparatively carbon deficient)
star that was probably enriched by an asymptotic branch giant (AGB)
star (see Gacrux) but is now a very dim,
white dwarf companion, which has an observed separation of around 4,400 AUs — 5.7» at a HIPPARCOS distance estimate of 42.0 ly (Porto de Mello and da Silva, 1997; and Poveda et al, 1993, pp. 74 - 75).