Share
High Energy Particle Acceleration and Turbulent Magnetic Field Amplification in Shell Type Supernova Remnants
National Aeronautics and Space Administr
(Author)
·
Jonathan Wilmore Keohane
(Author)
·
Biblioscholar
· Paperback
High Energy Particle Acceleration and Turbulent Magnetic Field Amplification in Shell Type Supernova Remnants - National Aeronautics and Space Administr ; Keohane, Jonathan Wilmore
Choose the list to add your product or create one New List
✓ Product added successfully to the Wishlist.
Go to My Wishlists
Origin: U.S.A.
(Import costs included in the price)
It will be shipped from our warehouse between
Monday, July 22 and
Monday, July 29.
You will receive it anywhere in United Kingdom between 1 and 3 business days after shipment.
Synopsis "High Energy Particle Acceleration and Turbulent Magnetic Field Amplification in Shell Type Supernova Remnants"
Thesis submitted to the faculty of the Graduate School of the University of Minnesota in partial fulfillment of the requirements for the degree of Doctor of Philosophy. Part I discusses the spatial correlation between the x-ray and radio morphologies of Cas A, and in the process address: the effect of inhomogeneous absorption on the apparent x-ray morphology, the interaction between the SNR and a molecular cloud, and the rapid move toward equipartition between the magnetic and gas energy densities. Discussions of the x-ray./radio correlation continues in Chapter 5, where we present a new, deep, ROSAT HRI image of Cas A. Chapter 7 presents ASCA spectra, with non-thermal spectral fits for 13 of the youngest SNRs in the Galaxy.
- 0% (0)
- 0% (0)
- 0% (0)
- 0% (0)
- 0% (0)
All books in our catalog are Original.
The book is written in English.
The binding of this edition is Paperback.
✓ Producto agregado correctamente al carro, Ir a Pagar.