Stan Owocki (University of Delaware)
Fundamentals of Astrophysics
Stan Owocki (University of Delaware)
Fundamentals of Astrophysics
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Designed for one-semester astrophysics courses, the second edition of this textbook is aimed at science and engineering students with college-level calculus-based physics. Bridging the gap between basic astronomy books and advanced astrophysics texts, it offers an overview of stars, exoplanets, the interstellar medium, galaxies, and cosmology.
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Designed for one-semester astrophysics courses, the second edition of this textbook is aimed at science and engineering students with college-level calculus-based physics. Bridging the gap between basic astronomy books and advanced astrophysics texts, it offers an overview of stars, exoplanets, the interstellar medium, galaxies, and cosmology.
Produktdetails
- Produktdetails
- Verlag: Cambridge University Press
- 2 Revised edition
- Seitenzahl: 300
- Erscheinungstermin: 1. September 2025
- Englisch
- Abmessung: 240mm x 169mm x 19mm
- Gewicht: 620g
- ISBN-13: 9781009618007
- ISBN-10: 1009618008
- Artikelnr.: 73527889
- Herstellerkennzeichnung
- Libri GmbH
- Europaallee 1
- 36244 Bad Hersfeld
- gpsr@libri.de
- Verlag: Cambridge University Press
- 2 Revised edition
- Seitenzahl: 300
- Erscheinungstermin: 1. September 2025
- Englisch
- Abmessung: 240mm x 169mm x 19mm
- Gewicht: 620g
- ISBN-13: 9781009618007
- ISBN-10: 1009618008
- Artikelnr.: 73527889
- Herstellerkennzeichnung
- Libri GmbH
- Europaallee 1
- 36244 Bad Hersfeld
- gpsr@libri.de
Stan Owocki is an Emeritus Professor within the Department of Physics and Astronomy at the University of Delaware. He received his Ph.D. from the University of Colorado in 1982 and had post-doctoral positions at Harvard University and University of California, San Diego before joining the faculty at U. Delaware in 1987. Co-author of more than 300 scientific papers, his research focuses on mass loss from luminous, massive stars. He has extensive experience of teaching at both the undergraduate and graduate levels, with his flagship "Fundamentals of Astrophysics" course laying the foundation for this text.
Part I. Stellar Properties: 1. Introduction
2. Astronomical distances
3. Stellar luminosity
4. Surface temperature from a star's color
5. Stellar radius from luminosity and temperature
6. Composition and ionization from stellar spectra
7. Surface gravity and escape/orbital speed
8. Stellar ages and lifetimes
9. Stellar space velocities
10. Using binary systems to determine masses and radii
11. Stellar rotation
12. Light intensity and absorption
13. Observational methods
14. Our Sun
Part II. Stellar Structure and Evolution: 15. Hydrostatic balance between pressure and gravity
16. Transport of radiation from interior to surface
17. Structure of radiative versus convective stellar envelopes
18. Hydrogen fusion and the mass range of stars
19. Post-main-sequence evolution: low-mass stars
20. Post-main-sequence evolution: high-mass stars
Part III. Interstellar Medium and Formation of Stars and Planets: 21. The interstellar medium
22. Star formation
23. Origin of planetary systems
24. Water planet Earth
25. Extra-solar planets
Part IV. Our Milky Way and Other Galaxies
26. Our Milky Way galaxy
27. External galaxies
28. Active galactic nuclei and quasars
29. Large-scale structure and galaxy formation and evolution
Part V. Cosmology: 30. Newtonian dynamical model of universe expansion
31. Accelerating universe with a cosmological constant
32. The hot Big Bang
33. Eras in the evolution of the universe
Appendices
Index.
2. Astronomical distances
3. Stellar luminosity
4. Surface temperature from a star's color
5. Stellar radius from luminosity and temperature
6. Composition and ionization from stellar spectra
7. Surface gravity and escape/orbital speed
8. Stellar ages and lifetimes
9. Stellar space velocities
10. Using binary systems to determine masses and radii
11. Stellar rotation
12. Light intensity and absorption
13. Observational methods
14. Our Sun
Part II. Stellar Structure and Evolution: 15. Hydrostatic balance between pressure and gravity
16. Transport of radiation from interior to surface
17. Structure of radiative versus convective stellar envelopes
18. Hydrogen fusion and the mass range of stars
19. Post-main-sequence evolution: low-mass stars
20. Post-main-sequence evolution: high-mass stars
Part III. Interstellar Medium and Formation of Stars and Planets: 21. The interstellar medium
22. Star formation
23. Origin of planetary systems
24. Water planet Earth
25. Extra-solar planets
Part IV. Our Milky Way and Other Galaxies
26. Our Milky Way galaxy
27. External galaxies
28. Active galactic nuclei and quasars
29. Large-scale structure and galaxy formation and evolution
Part V. Cosmology: 30. Newtonian dynamical model of universe expansion
31. Accelerating universe with a cosmological constant
32. The hot Big Bang
33. Eras in the evolution of the universe
Appendices
Index.
Part I. Stellar Properties: 1. Introduction
2. Astronomical distances
3. Stellar luminosity
4. Surface temperature from a star's color
5. Stellar radius from luminosity and temperature
6. Composition and ionization from stellar spectra
7. Surface gravity and escape/orbital speed
8. Stellar ages and lifetimes
9. Stellar space velocities
10. Using binary systems to determine masses and radii
11. Stellar rotation
12. Light intensity and absorption
13. Observational methods
14. Our Sun
Part II. Stellar Structure and Evolution: 15. Hydrostatic balance between pressure and gravity
16. Transport of radiation from interior to surface
17. Structure of radiative versus convective stellar envelopes
18. Hydrogen fusion and the mass range of stars
19. Post-main-sequence evolution: low-mass stars
20. Post-main-sequence evolution: high-mass stars
Part III. Interstellar Medium and Formation of Stars and Planets: 21. The interstellar medium
22. Star formation
23. Origin of planetary systems
24. Water planet Earth
25. Extra-solar planets
Part IV. Our Milky Way and Other Galaxies
26. Our Milky Way galaxy
27. External galaxies
28. Active galactic nuclei and quasars
29. Large-scale structure and galaxy formation and evolution
Part V. Cosmology: 30. Newtonian dynamical model of universe expansion
31. Accelerating universe with a cosmological constant
32. The hot Big Bang
33. Eras in the evolution of the universe
Appendices
Index.
2. Astronomical distances
3. Stellar luminosity
4. Surface temperature from a star's color
5. Stellar radius from luminosity and temperature
6. Composition and ionization from stellar spectra
7. Surface gravity and escape/orbital speed
8. Stellar ages and lifetimes
9. Stellar space velocities
10. Using binary systems to determine masses and radii
11. Stellar rotation
12. Light intensity and absorption
13. Observational methods
14. Our Sun
Part II. Stellar Structure and Evolution: 15. Hydrostatic balance between pressure and gravity
16. Transport of radiation from interior to surface
17. Structure of radiative versus convective stellar envelopes
18. Hydrogen fusion and the mass range of stars
19. Post-main-sequence evolution: low-mass stars
20. Post-main-sequence evolution: high-mass stars
Part III. Interstellar Medium and Formation of Stars and Planets: 21. The interstellar medium
22. Star formation
23. Origin of planetary systems
24. Water planet Earth
25. Extra-solar planets
Part IV. Our Milky Way and Other Galaxies
26. Our Milky Way galaxy
27. External galaxies
28. Active galactic nuclei and quasars
29. Large-scale structure and galaxy formation and evolution
Part V. Cosmology: 30. Newtonian dynamical model of universe expansion
31. Accelerating universe with a cosmological constant
32. The hot Big Bang
33. Eras in the evolution of the universe
Appendices
Index.







