62,69 €
Structure and Evolution of Single Stars
Structure and Evolution of Single Stars
  • Sold out
Structure and Evolution of Single Stars
Structure and Evolution of Single Stars
El. knyga:
62,69 €
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…
0

Structure and Evolution of Single Stars (e-book) (used book) | bookbook.eu

Reviews

(2.00 Goodreads rating)
Rate it too! All reviews

Description

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.

62,69 €
Log in and for this item
you will receive 0,63 Book Euros! ?

Electronic book:
Delivery after ordering is instant! Intended for reading only on a computer, tablet or other electronic device.

Lowest price in 30 days: 62,09 €

Lowest price recorded: 2025-09-27 17:20:04


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.

Reviews

  • No reviews
0 customers have rated this item.
5
0%
4
0%
3
0%
2
0%
1
0%
(will not be displayed)