Non-radial oscillations and vibrational stability of massive stars initially composed of pure hydrogen
| dc.contributor.author | Wan Fook Sun | |
| dc.date.accessioned | 2017-12-06T03:36:35Z | |
| dc.date.available | 2017-12-06T03:36:35Z | |
| dc.date.copyright | 1966 | |
| dc.date.issued | 1966 | |
| dc.date.updated | 2017-11-22T22:12:55Z | |
| dc.description.abstract | The study of vibrational stability of nassive stars undergoing radial oscillations has been investigated thoroughly by Schwarzschild and Harm [1], A. Boury [2] and P. Ledoux [3]. However, until recentl~ very little work has been done on the stability of stars undergoing non-radial oscillations. R.L. Simon [4] has studied the vibrational stability of the standard model undergoing non-radial oscillations but the difficulty in solving the basic equations governing non-radial oscillations has hampered the study of the stability of massive stars. | en_AU |
| dc.format.extent | 1 v | |
| dc.identifier.other | b1016124 | |
| dc.identifier.uri | http://hdl.handle.net/1885/137009 | |
| dc.language.iso | en | en_AU |
| dc.subject.lcsh | Oscillations | |
| dc.subject.lcsh | Vibration | |
| dc.title | Non-radial oscillations and vibrational stability of massive stars initially composed of pure hydrogen | en_AU |
| dc.type | Thesis (PhD) | en_AU |
| dcterms.valid | 1966 | en_AU |
| local.contributor.affiliation | Department of Mathematics, The Australian National University | en_AU |
| local.contributor.supervisor | Van der Borght, R. | |
| local.description.notes | Thesis (Ph.D.)--Australian National University, 1966. This thesis has been made available through exception 200AB to the Copyright Act. | en_AU |
| local.identifier.doi | 10.25911/5d70ecfd0bd47 | |
| local.identifier.proquest | Yes | |
| local.mintdoi | mint | |
| local.type.degree | Doctor of Philosophy (PhD) | en_AU |
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