randa177
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Can anybody explain to me what a Pop. I object is?
The discussion centers around the classification of stars into Population I and Population II, exploring their characteristics, formation, and distribution within the Milky Way galaxy. Participants examine the distinctions based on metallicity, age, and spatial distribution, as well as the implications of these classifications in astrophysics.
Participants express various viewpoints on the definitions and characteristics of Population I and II stars, indicating that multiple competing views remain and the discussion is not resolved.
Some limitations include the lack of consensus on the precise metallicity cutoff between Population I and II stars, as well as the dependence on definitions of terms like "metallicity" and "star formation." Unresolved aspects of the discussion include the implications of these classifications for understanding stellar evolution.
So where is the cutoff between Pop I and Pop II in terms of metallicity? 0.1% or 1% metals?astronomy.osu.edu said:17.4 POPULATION I
The two stellar populations differ from each other in spatial distribution, age, and composition.
Features of Population I:
• occurs in disk
• old and young stars
• open clusters (and isolated/binary stars)
• roughly solar metallicity
[typical composition 70% hydrogen, 28% helium, 2% metals]
Associated with Population I:
• interstellar gas and dust
• star-forming gas clouds
• Type II supernovae
17.5 POPULATION II
Features of Population II:
• occurs in spheroid, especially the stellar halo
• old stars only (no blue main sequence stars)
• globular clusters (and isolated/binary stars)
• low metallicity, 1/1000 to 1/100 solar
[typical composition 75% hydrogen, 24.99% helium, 0.01% metals]
Associated with Population II:
• very little interstellar gas or dust
• no star formation
• only Type I supernovae