Stellar atmosphere

  • #1
how can i calculate the fractional abundance of HI, HII, H- and e- for hydrogen in the photosphere (T=5770K) and density 10^17?
 

Answers and Replies

  • #2
2
0
Analysis of spectrum lines, A stronger line in a particular location means there is alot of that substance to absorb at that particular wavelength.
 

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