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Stan Owocki Fundamentals of Astrophysics Chapter 6: Composition and Ionization from Stellar Spectra 6.1 Spectral line absorption and emission 6.2 Elemental composition of the Sun and stars 6.3 Stellar spectral type 6.4 Hertzsprung-Russell (H-R) diagram 6.5 Questions and exercises I Stellar Properties

Fundamentals of Astrophysics - University of Delaware

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Page 1: Fundamentals of Astrophysics - University of Delaware

Stan OwockiFundamentals of Astrophysics

Chapter 6: Composition and Ionization from Stellar Spectra

6.1 Spectral line absorption and emission6.2 Elemental composition of the Sun and stars 6.3 Stellar spectral type6.4 Hertzsprung-Russell (H-R) diagram6.5 Questions and exercises

I Stellar Properties

Page 2: Fundamentals of Astrophysics - University of Delaware

Sun’s spectrum

Page 3: Fundamentals of Astrophysics - University of Delaware

Continuum vs. line emission/absorption

Page 4: Fundamentals of Astrophysics - University of Delaware

Hydrogen atom

Energy levels

emission line spectrum=>

absorption line spectrum=>

Lyman series

Balmer series

Paschen series

Page 5: Fundamentals of Astrophysics - University of Delaware

Bohr atom

Page 6: Fundamentals of Astrophysics - University of Delaware

Elemental Abundances

by number:

by mass:

Page 7: Fundamentals of Astrophysics - University of Delaware

Sequence of spectral types

Page 8: Fundamentals of Astrophysics - University of Delaware

Hertzsprung-Russell diagram

Page 9: Fundamentals of Astrophysics - University of Delaware

Observed H-R diagram from Gaia satellite

Page 10: Fundamentals of Astrophysics - University of Delaware

Ch. 6 Quick Questions