How such a dense planet formed is unclear, the researchers say, but it's probably the crystalline vestige
of a white dwarf star whose atmosphere was stripped away by the parent pulsar.
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.
Not exact matches
The researchers found that relatively cool accretion discs around young
stars,
whose inner edges can be several times the size
of the Sun, show the same behaviour as the hot, violent accretion discs around planet - sized
white dwarfs, city - sized black holes and supermassive black holes as large as the entire Solar system, supporting the universality
of accretion physics.
A Southampton astronomer is among a team
of international researchers
whose work has revealed a surprising similarity between the way in which astronomical objects grow including black holes,
white dwarfs and young
stars.
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.
The giants among those
stars are presumed to produce this carbon themselves, but some
stars in this class are double
stars,
whose odd atmosphere is suspected
of having been transferred from a companion that is now a
white dwarf, when the companion was a carbon -
star.