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Structure and Evolution of Single Stars
139,22 € 
- Mēs nosūtīsim 10-14 darba dienu laikā.
Structure and Evolution of Single Stars: An introduction is intended for upper-level undergraduates and beginning graduates with a background in physics. Following a brief overview of the background observational material, the basic equations describing the structure and evolution of single stars are derived. The relevant physical processes, which include the equation of state, opacity, nuclear reactions and neutrino losses are then reviewed. Subsequent chapters describe the evolution of low-ma…
139.22
2025-06-02 08:00:00
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- Autors: James Macdonald
- Izdevējs MORGAN & CLAYPOOL
- Gads: 2015
- Lapas: 188
- ISBN-10 : 1681740419
- ISBN-13 : 9781681740416
- Formāts: 17.8 x 25.4 x 1 cm, minkšti viršeliai
- Valoda: Anglų
- Extra -10% atlaide, ievadot kodu: EXTRA
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Structure and Evolution of Single Stars: An introduction is intended for upper-level undergraduates and beginning graduates with a background in physics. Following a brief overview of the background observational material, the basic equations describing the structure and evolution of single stars are derived. The relevant physical processes, which include the equation of state, opacity, nuclear reactions and neutrino losses are then reviewed. Subsequent chapters describe the evolution of low-mass stars from formation to the final white dwarf phase. The final chapter deals with the evolution of massive stars.10 EXTRA % atlaide
139,22 €
154,69 €
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- Autors: James Macdonald
- Izdevējs MORGAN & CLAYPOOL
- Gads: 2015
- Lapas: 188
- ISBN-10: 1681740419
- ISBN-13: 9781681740416
- Formāts 17.8 x 25.4 x 1 cm, minkšti viršeliai
- Valoda: Anglų
Structure and Evolution of Single Stars: An introduction is intended for upper-level undergraduates and beginning graduates with a background in physics. Following a brief overview of the background observational material, the basic equations describing the structure and evolution of single stars are derived. The relevant physical processes, which include the equation of state, opacity, nuclear reactions and neutrino losses are then reviewed. Subsequent chapters describe the evolution of low-mass stars from formation to the final white dwarf phase. The final chapter deals with the evolution of massive stars.
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