| dc.contributor.advisor | Ray, Tom | |
| dc.contributor.author | Gras-Velázquez, Àgueda | |
| dc.date.accessioned | 2019-04-30T08:56:17Z | |
| dc.date.available | 2019-04-30T08:56:17Z | |
| dc.date.issued | 2006 | |
| dc.identifier.citation | Àgueda Gras-Velázquez, 'Disks around weak-line T Tauri stars', [thesis], Trinity College (Dublin, Ireland). School of Physics, 2006, pp 162 | |
| dc.identifier.other | THESIS 8263 | |
| dc.description.abstract | The formation of low -mass (M ~ 1 M⊙) stars has generally been divided into four
stages before reaching the main sequence: Class 0 (cloud of gas and dust) -> Class I
(embedded star with disk in envelope) -> Class II (visible star with disk ) -> Class III
(visible star with no disk). Classical T Tauri stars (CTTS ) are associated to the Class II
stage while Weak-line T Tauri stars (WTTS ) with the Class III stage. | |
| dc.format | 1 volume | |
| dc.language.iso | en | |
| dc.publisher | Trinity College (Dublin, Ireland). School of Physics | |
| dc.relation.isversionof | http://stella.catalogue.tcd.ie/iii/encore/record/C__Rb12986314 | |
| dc.subject | Physics, Ph.D. | |
| dc.subject | Ph.D. Trinity College Dublin | |
| dc.title | Disks around weak-line T Tauri stars | |
| dc.type | thesis | |
| dc.type.supercollection | thesis_dissertations | |
| dc.type.supercollection | refereed_publications | |
| dc.type.qualificationlevel | Doctoral | |
| dc.type.qualificationname | Doctor of Philosophy (Ph.D.) | |
| dc.rights.ecaccessrights | openAccess | |
| dc.format.extentpagination | pp 162 | |
| dc.description.note | TARA (Trinity's Access to Research Archive) has a robust takedown policy. Please contact us if you have any concerns: rssadmin@tcd.ie | |
| dc.identifier.uri | http://hdl.handle.net/2262/86350 | |
