Further to jake's helioseismologically correct answer, proto stars that don't quite make it to the size of our own sun ( 1 Msun ) in mass, become brown dwarfs Stars are classified in relation to their temperature and luminosity. Our own sun is a star classified as a spectral class G2 and its luminosity as class V .
By the way, some stars do (generally termed Massive Stars) (more than about 30 times the mass of our own sun) "burn up" quite quickly... some in less than a million years and when they "die" are now thought to be one of the two sources for the observed gamma ray bursts throughout the universe...