Many stars which are members of an open cluster are blue, hot stars, with relatively short life expectancies (a few hundred thousand years to a couple of million years life).
The HR diagram does not reference stars on their way to the main sequence, only during or after.
The temperature and luminosity of stars.
It shows certain key characteristics (brightness, and temperature) of stars.
I don't know ok
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 contains only stars - so everywhere.
Several regions of the HR diagram have been given names, although stars can occupy any portion. The brightest stars are called supergiants. Star clusters are rich in stars just off the main sequence called red giants. Main sequence stars are called dwarfs.
Of course they are on the HR diagram. They are simply not on the main sequence.
All stars.
main-sequence stars
The main reason that the HR Diagram is so useful and important to scientists is, you can tell the size of the star by plotting it on the HR Diagram. The different sizes of stars form a pattern on the HR diagram.
stars there called stars
stars there called stars
The red dwarves.
Main sequence
They are very hot stars.
The HR diagram does not reference stars on their way to the main sequence, only during or after.