The Hertzsprung--Russell diagram is a scatter graph of stars showing the relationship between the stars' absolute magnitudes or luminosities versus their spectral types or classifications and effective temperatures.
Because the luminosity is low or non existent in the case of black holes, they do not appear on the HR diagram.
The Hertzsprung--Russell diagram is a scatter graph of stars showing the relationship between the stars' absolute magnitudes or luminosities versus their spectral types or classifications and effective temperatures.Because the luminosity is low or non existent in the case of black holes, they do not appear on the HR diagram.
Neutron stars and black holes.
Most stars end up as white dwarfs. A few become neutron stars. Even fewer become black holes.
neutron stars and black holes
Only in that they where formed by the same process. A neutron star formed from a star with less mass than a black hole
The Hertzsprung--Russell diagram is a scatter graph of stars showing the relationship between the stars' absolute magnitudes or luminosities versus their spectral types or classifications and effective temperatures.Because the luminosity is low or non existent in the case of black holes, they do not appear on the HR diagram.
Black holes, neutron stars, and the white dwarfs
See related
Neutron stars and black holes.
black holes and neutron stars
Black Holes are the most dense. Second to black holes would be Neutron Stars
Some massive stars will become neutron stars. When massive stars die they will either become neutron stars or black holes depending on how much mass is left behind.
'Black holes' and neutron stars.
Most stars end up as white dwarfs. A few become neutron stars. Even fewer become black holes.
No. They do not have enough mass to become black holes. Depending on the mass they will either become white dwarfs or neutron stars.
neutron stars and black holes
No. Blue stars will generally leave behind neutron stars or black holes.