The luminosity of a white dwarf star can vary depending on its mass and age, but typically ranges from about 0.001 to 0.1 times the luminosity of the Sun. These stars are small and dense, with surface temperatures ranging from 8,000 to 100,000 Kelvin, which affects their brightness.
Depending on the distance between the binary pair, it is possible for the white dwarf to draw gas from it's companion causing the star to reach the Chandrasekhar limit causing the white dwarf to explode as a nova or a type La supernova.
A cooled white dwarf is a black dwarf. I think you are thinking of a neutron star which has nothing to do with a white dwarf.
A white dwarf.A white dwarf.A white dwarf.A white dwarf.
A white dwarf could not become a red dwarf. A white dwarf is a remnant of a dead star. A red dwarf is a star with a very low mass.
No. A white dwarf is the remnant of a low to medium mass star.
A white dwarf.A white dwarf.A white dwarf.A white dwarf.
A white dwarf.A white dwarf.A white dwarf.A white dwarf.
A white dwarf.A white dwarf.A white dwarf.A white dwarf.
A white dwarf.A white dwarf.A white dwarf.A white dwarf.
A white dwarf.A white dwarf.A white dwarf.A white dwarf.
A blue dwarf star would have high temperature and low luminosity in the Hertzsprung-Russell (HR) diagram. Blue dwarf stars are in the lower left corner of the diagram, characterized by their high surface temperature and faint luminosity compared to other stars of similar temperature.
No. A dwarf star is a small star. A white dwarf is just one particular type of dwarf star, but there are other types.
Depending on the distance between the binary pair, it is possible for the white dwarf to draw gas from it's companion causing the star to reach the Chandrasekhar limit causing the white dwarf to explode as a nova or a type La supernova.
No a white dwarf is a small compact star.
A cooled white dwarf is a black dwarf. I think you are thinking of a neutron star which has nothing to do with a white dwarf.
A white dwarf.A white dwarf.A white dwarf.A white dwarf.
A white dwarf diagram typically shows the main features of a star in the final stage of its life cycle, including its small size, high density, and cooling temperature. It may also display the relationship between luminosity and temperature as the star evolves.