Observation and Analysis of Stellar Photospheres
portes grátis
Observation and Analysis of Stellar Photospheres
Gray, David F.
Cambridge University Press
12/2021
550
Mole
Inglês
9781009078016
15 a 20 dias
842
Descrição não disponível.
Preface to the first edition; Preface to the second edition; Preface to the third edition; Preface to the fourth edition; 1. Background; 2. Fourier transforms; 3. Spectroscopic tools; 4. Light detectors; 5. Radiation terms and definitions; 6. The black body and its radiation; 7. Energy transport in stellar photospheres; 8. The continuous absorption coefficient; 9. The model photosphere; 10. Analysis of stellar continua; 11. The line absorption coefficient; 12. The measurement of spectral lines; 13. The behavior of spectral lines; 14. The measurement of stellar radii and temperatures; 15. The measurement of surface gravity; 16. The measurement of chemical composition; 17. Velocity fields in stellar photospheres; 18. Stellar rotation; Appendix A. Useful constants; Appendix B: Approximate physical parameters of stars; Appendix C. Atomic data; Appendix D. The strongest lines in the solar spectrum; Appendix E. Computation of random errors; Index.
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Preface to the first edition; Preface to the second edition; Preface to the third edition; Preface to the fourth edition; 1. Background; 2. Fourier transforms; 3. Spectroscopic tools; 4. Light detectors; 5. Radiation terms and definitions; 6. The black body and its radiation; 7. Energy transport in stellar photospheres; 8. The continuous absorption coefficient; 9. The model photosphere; 10. Analysis of stellar continua; 11. The line absorption coefficient; 12. The measurement of spectral lines; 13. The behavior of spectral lines; 14. The measurement of stellar radii and temperatures; 15. The measurement of surface gravity; 16. The measurement of chemical composition; 17. Velocity fields in stellar photospheres; 18. Stellar rotation; Appendix A. Useful constants; Appendix B: Approximate physical parameters of stars; Appendix C. Atomic data; Appendix D. The strongest lines in the solar spectrum; Appendix E. Computation of random errors; Index.
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