Thompson, Alan McLure
(1986)
Energy Transport in Radially Accreting White Dwarf Stars.
PhD thesis, University of Glasgow.
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Abstract
AM Herculis stars form a subclass of cataclysmic variables, the defining characteristic of which is that they possess a high degree of polarisation at optical frequencies. Physically they have two notable features. Firstly, the white dwarf star has a sufficiently high magnetic field (B ~ 10.
| Item Type: |
Thesis
(PhD)
|
| Qualification Level: |
Doctoral |
| Keywords: |
Astronomy |
| Date of Award: |
1986 |
| Depositing User: |
Enlighten Team
|
| Unique ID: |
glathesis:1986-77426 |
| Copyright: |
Copyright of this thesis is held by the author. |
| Date Deposited: |
14 Jan 2020 09:08 |
| Last Modified: |
14 Jan 2020 09:08 |
| URI: |
http://theses.gla.ac.uk/id/eprint/77426 |
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