It appears you're describing a diagram related to the Hertzsprung-Russell (H-R) diagram, which is a scatter plot of stars showing the relationship between their absolute magnitudes or luminosities versus their stellar classifications or effective temperatures.
In the H-R diagram:
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Main Sequence Stars: Most stars, including our Sun, are found on the main sequence, which runs diagonally from the upper left (hot, luminous stars) to the lower right (cooler, dim stars). These stars are in the stable phase of hydrogen burning in their cores.
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Giants: Above the main sequence, we find giant stars, which are larger and more luminous than main sequence stars of similar temperature. These stars have exhausted the hydrogen in their cores and have expanded.
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White Dwarfs: Below the main sequence, on the lower left of the diagram, are white dwarfs, which are remnants of stars that have exhausted their nuclear fuel. These stars are very hot but not very luminous due to their small size.
In summary, the classification you mentioned aligns with the typical structure of the H-R diagram, emphasizing that the majority of stars are found in the main sequence category. If you have a specific question about this diagram or need further details, feel free to ask!