The central stars of planetary nebulae are the hottest known
stars. They have been detected with surface temperatures up to
250,000 K. One example of a planetary nebula with such a hot
central star is NGC 2240. At such high temperatures, most of the
radiation is emitted in the ultraviolet part of the spectrum so the
star is often not obvious in visual images of the nebula.
Planetary nebulae form when evolved stars eject their outer
layers. Their central stars are what were the stellar cores and
their surface temperatures continues to rise after the nebulae
have formed. The maximum temperature reached is
predetermined by the mass of the stellar core. Masses are
thought to range between 0,55 and 1.2 times the Sun's mass.
The greater the mass, the higher the maximum surface
temperature achieved by the star.
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