In this thesis, a hydrodynamical model for the 2006 outburst of the recurrent nova RS Ophiuchi (RS Oph) has been created. RS Oph is a close binary system comprising a white dwarf (WD) and a red giant (RG).
| Identifer | oai:union.ndltd.org:bl.uk/oai:ethos.bl.uk:492764 |
| Date | January 2009 |
| Creators | Vaytet, Neil M. H. |
| Publisher | University of Manchester |
| Source Sets | Ethos UK |
| Detected Language | English |
| Type | Electronic Thesis or Dissertation |
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