Computational Star Formation (IAU S270)

Inbunden, Engelska, 2011

Del i serien Proceedings of the International Astronomical Union Symposia and Colloquia

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Beskrivning

The rapid advance of computer capabilities over the last two decades has opened up a new field of numerical simulations in which detailed physical models can be made to represent the most complex processes. IAU Symposium 270 reviews a wide range of topics relevant to computer modeling in the fields of interstellar gas dynamics, star formation and galactic dynamics. It includes numerical techniques for modeling physical processes such as self-gravitating, radiative magnetohydrodynamics, as well as novel hardware options for acceleration and a view into the future of computation. Observations of interstellar gas and star formation are also reviewed. This book is ideal for graduate students and researchers in the field of numerical astrophysics.

Produktinformation

Utgivningsdatum:2011-05-19
Mått:180 x 254 x 28 mm
Vikt:1 140 g
Format:Inbunden
Språk:Engelska
Serie:Proceedings of the International Astronomical Union Symposia and Colloquia
Antal sidor:574
Förlag:Cambridge University Press
ISBN:9780521766432

Utforska kategorier

Tillämpad fysik inom Naturvetenskap och teknik

Recensioner i media

'… excellent contributions, including papers that my students and [postdoctorates] would find interesting and relevant. Well worth a read if this is an area of interest.' The Observatory

Innehållsförteckning

1. Historical introduction; 2. Individual star formation: observations; 3. Low-mass star formation: observations; 4. Individual star formation: theory; 5. Formation of clusters: observations; 6. Formation of clusters: theory; 7. Numerical methods: MHD; 8. Numerical methods: radiative dynamics; 9. Local star formation processes; 10. Star formation feedback; 11. Star formation on galactic scales; 12. Special purpose hardware; 13. Computational methods; 14. Radiation diagnostics of star formation; 15. Large scale star formation; 16. Cosmological star formation; 17. Computational star formation: Summary; Index.