The Stars

5. The stellar core left behind after a dying star has exhausted its nuclear.
6. The sequence of thermonuclear reactions that provides most of its energy radiation by hotter stars.
8. Lies in the last stage of stellar evolution.
10. The density of matter is so high that electrons cannot be packed closer together.
13. The maximum mass which a star near the end of its life cycle can become a white dwarf.
14. A rotating neutron stars observed to have pulses of radiation at very regular intervals.

1. A way of representing data using 0s and 1s.
2. A region of cosmic gas and dust formed from the cast of outer layers of a dying star.
3. When the density of matter is so high that neutrons cannot be packed.
4. The neutron stars with ridiculously, powerful magnetic fields.
7. Conserved when there is zero net torque applied a system, where the system is the object.
9. The colossal explosion of a star.
11. A star showing a sudden large increase in brightness and then slowly returning to its original state.
12. Stars with mass less than about 2 times the mass of the sun.