Based on initial size and chemical composition a star will enter a band on the HR diagram as a mains sequence star. Stars on the main sequence are in equilibrium from thermal pressure trying to enlarge the star and gravitational pressure trying to collapse the star. Stars on the main sequence range from massive hot blue-white stars to much less massive red stars.
The HR diagram does not reference stars on their way to the main sequence, only during or after.
above the main-sequence stars
main sequence
A main-sequence star is one that is along a curve where the majority of stars are located, when plotted in an H-R diagram. It is a star that gets its energy from fusing hydrogen-1 into helium-4.
The main sequence - the region across the middle of the diagram.
Main sequence stars.
The HR diagram does not reference stars on their way to the main sequence, only during or after.
I assume the different points on the main sequence represent a kind of balance for the case of hydrogen-to-helium fusion.
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
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.
As the HR diagram shows, the hottest stars on the main sequence range from 30,000K as blue-white stars to about 3,000K as redish stars.
main sequence