dc.contributor.advisor |
Gallo, Luigi C. |
|
dc.creator |
Gonzalez, Adam G. |
|
dc.date.accessioned |
2021-09-02T16:11:22Z |
|
dc.date.available |
2021-09-02T16:11:22Z |
|
dc.date.issued |
2021 |
|
dc.identifier.uri |
http://library2.smu.ca/xmlui/handle/01/29819 |
|
dc.description |
1 online resource (x, 250 pages) : illustrations, charts (some colour), graphs (some colour) |
|
dc.description |
Includes abstract and appendices. |
|
dc.description |
Includes bibliographic references (pages 242-250). |
|
dc.description.abstract |
High-velocity outflows in active galactic nuclei usually manifest as either a collimated
jet or diffuse wind. These outflows carry a significant amount of energy from the central
environment surrounding the supermassive black hole into the host galaxy, potentially altering the course of star formation therein. Our current understanding of how these outflows
relate to the central engine, however, remains incomplete. We do not know why some active
galactic nuclei exhibit jets, why some have winds, how either outflow responds to changes
in the conditions of the X-ray emitting region, and if the ones that have no outflows are
intrinsically different systems. In Chapters 2 and 3, I present case studies of two radio-loud
active galaxies with jets, III Zw 2 and IRAS 17020+4544, in an effort to explore the postulated disc-jet connection in such systems using X-ray observations. Spectral and variability
properties in each source suggest that an outflowing X-ray source may act as the jet base.
In a future work, this interpretation will be explored using a sample of both radio-loud
and radio-quiet sources to test its validity. A sample of 20 active galaxies that have been
previously reported as exhibiting ultra-fast winds in their X-ray spectra is used to probe
what underlying driving mechanisms may produce such outflows, as well as how the outflow
properties relate to the conditions of the central engine. We find that wind properties are
closely linked to a variety of source parameters, such as accretion rate and disc inclination
angle. The properties of six extreme accretors may suggest non-standard accretion disc scenarios for which no wind is necessary, highlighting the need to explore alternative models.
Future X-ray missions with enhanced spectral resolution will enable more accurate determinations on the energetics and locations of these extreme winds, which are ill-constrained
with current data. |
en_CA |
dc.description.provenance |
Submitted by Greg Hilliard (greg.hilliard@smu.ca) on 2021-09-02T16:11:22Z
No. of bitstreams: 1
Gonzalez_Adam_PHD_2021.pdf: 25152220 bytes, checksum: 5b9bfd2d0bbb26d4cdbeb3e29954dfb0 (MD5) |
en |
dc.description.provenance |
Made available in DSpace on 2021-09-02T16:11:22Z (GMT). No. of bitstreams: 1
Gonzalez_Adam_PHD_2021.pdf: 25152220 bytes, checksum: 5b9bfd2d0bbb26d4cdbeb3e29954dfb0 (MD5)
Previous issue date: 2021-08-10 |
en |
dc.language.iso |
en |
en_CA |
dc.publisher |
Halifax, N.S. : Saint Mary's University |
|
dc.subject.lcsh |
Active galactic nuclei |
|
dc.subject.lcsh |
X-ray astronomy |
|
dc.subject.lcsh |
Bipolar outflows (Astrophysics) |
|
dc.subject.lcsh |
Galaxies -- Spectra |
|
dc.title |
Probing high-velocity outflows in active galactic nuclei and their relationship to the inner disc environment with X-ray observations |
en_CA |
dc.type |
Text |
en_CA |
thesis.degree.name |
Doctor of Philosophy in Astronomy |
|
thesis.degree.level |
Doctoral |
|
thesis.degree.discipline |
Astronomy and Physics |
|
thesis.degree.grantor |
Saint Mary's University (Halifax, N.S.) |
|