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Introduction to Stellar Structure
In the first part of this book, the author presents the basic properties of the stellar interior and describes them thoroughly, along with deriving the main stellar structure equations of temperature, density, pressure and luminosity, among others. The process and application of solving these equati...
| Clasificación: | Libro Electrónico |
|---|---|
| Autor principal: | |
| Autor Corporativo: | |
| Formato: | Electrónico eBook |
| Idioma: | Inglés |
| Publicado: |
Cham :
Springer International Publishing : Imprint: Springer,
2016.
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| Edición: | 1st ed. 2016. |
| Colección: | Astronomy and Planetary Sciences,
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| Temas: | |
| Acceso en línea: | Texto Completo |
MARC
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| 001 | 978-3-319-16142-6 | ||
| 003 | DE-He213 | ||
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| 008 | 150916s2016 sz | s |||| 0|eng d | ||
| 020 | |a 9783319161426 |9 978-3-319-16142-6 | ||
| 024 | 7 | |a 10.1007/978-3-319-16142-6 |2 doi | |
| 050 | 4 | |a QB1-991 | |
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| 100 | 1 | |a Maciel, Walter J. |e author. |4 aut |4 http://id.loc.gov/vocabulary/relators/aut | |
| 245 | 1 | 0 | |a Introduction to Stellar Structure |h [electronic resource] / |c by Walter J. Maciel. |
| 250 | |a 1st ed. 2016. | ||
| 264 | 1 | |a Cham : |b Springer International Publishing : |b Imprint: Springer, |c 2016. | |
| 300 | |a XV, 215 p. |b online resource. | ||
| 336 | |a text |b txt |2 rdacontent | ||
| 337 | |a computer |b c |2 rdamedia | ||
| 338 | |a online resource |b cr |2 rdacarrier | ||
| 347 | |a text file |b PDF |2 rda | ||
| 490 | 1 | |a Astronomy and Planetary Sciences, |x 2366-0090 | |
| 505 | 0 | |a Physical Properties of the Stars -- Physical Conditions in the Stellar Interior -- The Electron Gas -- The Photon Gas -- Adiabatic Processes in the Stellar Interior -- Polytropes -- Radiative Equilibrium -- Opacity -- Electron Conduction -- Convection -- Thermonuclear Reactions -- Energy Production -- Calculation of the Stellar Structure -- Appendix A: Constants and Units -- Solutions. | |
| 520 | |a In the first part of this book, the author presents the basic properties of the stellar interior and describes them thoroughly, along with deriving the main stellar structure equations of temperature, density, pressure and luminosity, among others. The process and application of solving these equations is explained, as well as linking these results with actual observations. The second part of the text describes what happens to a star over time, and how to determine this by solving the same equations at different points during a star's lifetime. The fate of various stars is quite different depending on their masses, and this is described in the final parts of the book. This text can be used for an upper level undergraduate course or an introductory graduate course on stellar physics. | ||
| 650 | 0 | |a Astronomy. | |
| 650 | 1 | 4 | |a Astronomy, Cosmology and Space Sciences. |
| 710 | 2 | |a SpringerLink (Online service) | |
| 773 | 0 | |t Springer Nature eBook | |
| 776 | 0 | 8 | |i Printed edition: |z 9783319161419 |
| 776 | 0 | 8 | |i Printed edition: |z 9783319161433 |
| 776 | 0 | 8 | |i Printed edition: |z 9783319366104 |
| 830 | 0 | |a Astronomy and Planetary Sciences, |x 2366-0090 | |
| 856 | 4 | 0 | |u https://doi.uam.elogim.com/10.1007/978-3-319-16142-6 |z Texto Completo |
| 912 | |a ZDB-2-PHA | ||
| 912 | |a ZDB-2-SXP | ||
| 950 | |a Physics and Astronomy (SpringerNature-11651) | ||
| 950 | |a Physics and Astronomy (R0) (SpringerNature-43715) | ||