Main Sequence Rules: Definition & Interpretation

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SUMMARY

The main sequence in an HR diagram is defined primarily by stars that are fusing hydrogen in their cores, categorized under luminosity class V. While the shaded area on the diagram may represent the main sequence, the distinction between main sequence stars and subgiants requires careful consideration of stellar interior models. Subgiants, which have ceased core fusion, are found between the main sequence and the red giant branch. Additionally, the presence of double or triple stars complicates the classification of stars on the HR diagram, as their combined spectra can obscure individual characteristics.

PREREQUISITES
  • Understanding of HR diagrams and stellar classification
  • Knowledge of stellar fusion processes, particularly hydrogen fusion
  • Familiarity with luminosity classes, specifically class V
  • Basic concepts of spectroscopic binaries and Doppler shifts
NEXT STEPS
  • Research stellar interior models to better understand the transition from main sequence to subgiants
  • Study the effects of binary star systems on HR diagram interpretations
  • Learn about the physical processes involved in stellar fusion and core evolution
  • Investigate the impact of orbital motion on parallax measurements in stellar distance calculations
USEFUL FOR

Astronomers, astrophysics students, and anyone interested in stellar evolution and classification will benefit from this discussion.

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When viewing an HR diagram, the main sequence curve is apparent, and the general shape of it is obvious. However, in this truncated version, it's unclear to me exactly which stars should be considered main sequence. I've added a shaded grey area as what I think I should count as main sequence, but there's a bit of room for interpretation. Are there hard-and-fast rules, or is it a matter of opinion? What do you think of this shaded area?
reddit help hr diagram.PNG
 
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There are two possible definitions of the main sequence, one is empirical and is the luminosity class V, but more commonly the definition is physical rather than empirical-- it is stars that are fusing hydrogen in their core. So if we take the latter meaning, the "subgiants" that are between the main sequence and the red giant branch have stopped core fusion and are instead fusing in small shells around an inert core, but the core is not yet tiny and degenerate. As the core shrinks further and goes degenerate, the shell gets really tiny and even higher in temperature, and the envelope will puff out and the star will move up and to the right into the giant branch. So I think you'd have to use interior models to decide where the main sequence ends and the subgiants begin, but your shaded area is probably the right ballpark.

Another key point to bear in mind is that many stars are actually double or triple stars, and this normally cannot be determined with certainty when the stars are plotted on the H-R diagram, unless you can separate the spectra based on their Doppler shifts for "spectroscopic" binaries (close binaries seen not from above the orbits). So you can get points that are actually a kind of average of different stellar types, creating confusion as to exactly what type of star you are looking at.
 
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Slightly OT: IIRC, a bunch of 'weird' Hipparchos distances have been attributed to orbital motion of unresolved binaries skewing the measured parallax. Some 'oops' seem due to mega-flares offsetting the nominal positions...

As mentioned above, spectroscopic binaries aligned such their orbital Doppler shifts are masked by surface activity are complex targets. Worse, contamination by mass-transfer or merger may skew determinations...

Must be said, watching such riddles and apparent paradoxes being patiently un-picked is excellent sport !
 

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