Because there not that hot
dwarf stars,giant stars,main sequence stars
The most massive main sequence stars are the brightest, (O main sequence star on Hertzsprung-Russel Diagram). Main sequence stars obey a mass-luminosity relation. On the H-R diagram the vertical axis is the brightness. So the stars along the top are the brightest (intrinsically).
Main-sequence stars
Main sequence
Of course they are on the HR diagram. They are simply not on the main sequence.
Main sequence stars.
The HR diagram does not reference stars on their way to the main sequence, only during or after.
In the HR-diagram, a diagram of color vs. luminosity, most stars are concentrated close to one curve, called the "main sequence". It turns out that stars on the main sequence are the stars that mainly get their energy by converting hydrogen into helium.
main-sequence stars
dwarf stars,giant stars,main sequence stars
After the main sequence, a star becomes a red giant.
The most massive main sequence stars are the brightest, (O main sequence star on Hertzsprung-Russel Diagram). Main sequence stars obey a mass-luminosity relation. On the H-R diagram the vertical axis is the brightness. So the stars along the top are the brightest (intrinsically).
above the main-sequence stars
Main-sequence stars
Main sequence
Of course they are on the HR diagram. They are simply not on the main sequence.
One of two groups of stars on the Hertzsprung -Russell diagram that have a different set of properties than the main sequence stars; bright, low-temperature giant stars that are enormously bright for their temperature.