Several newly
discovered white dwarf stars seem to have atmospheres consisting almost entirely of carbon.
Researchers have
discovered a white dwarf star with an atmosphere dominated by oxygen, a type of white dwarf that has been theorized to exist but not identified to date.
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.
Not exact matches
Astronomers have identified a
white dwarf star in our galaxy that may be the leftover remains of a recently
discovered type of supernova.
The first hint of the kamikaze asteroids came about 40 years ago, when astronomers
discovered heavy elements such as magnesium in the spectra of some
white dwarf stars.
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.
In 2003, astronomers announced that they had
discovered that iron from supernovae of the first
stars (possibly from Type Ia supernovae involving
white dwarfs) indicate that «massive chemically enriched galaxies formed» within one billion years after the Big Bang, and so the first
stars may have preceded the birth of supermassive black holes (more from Astronomy Picture of the Day, ESA, and Freudling et al, 2003).
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.