The application of hydrogen line photometry to Milky Way research
| dc.contributor.author | Graham, John Archibald | |
| dc.date.accessioned | 2017-12-11T03:57:31Z | |
| dc.date.available | 2017-12-11T03:57:31Z | |
| dc.date.copyright | 1963 | |
| dc.date.issued | 1963 | |
| dc.date.updated | 2017-11-22T22:30:26Z | |
| dc.format.extent | 125 leaves | |
| dc.identifier.other | b1649478 | |
| dc.identifier.uri | http://hdl.handle.net/1885/137461 | |
| dc.language.iso | en | en_AU |
| dc.subject.lcsh | Astronomical photometry | |
| dc.subject.lcsh | Stars Spectra | |
| dc.subject.lcsh | Milky Way | |
| dc.title | The application of hydrogen line photometry to Milky Way research | en_AU |
| dc.type | Thesis (PhD) | en_AU |
| dcterms.valid | 1963 | en_AU |
| local.contributor.affiliation | The Australian National University | en_AU |
| local.description.notes | Thesis (Ph.D.)--Australian National University, 1963. This thesis has been made available through exception 200AB to the Copyright Act. | en_AU |
| local.identifier.doi | 10.25911/5d6cf7f52ae27 | |
| local.identifier.proquest | Yes | |
| local.mintdoi | mint | |
| local.type.degree | Doctor of Philosophy (PhD) | en_AU |
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