Probing galaxies with quasar absorption lines

用类星体吸收线探测星系

• 批准号: 349730-2007
• 负责人: Ellison, Sara
• 金额: $ 1.46万
• 依托单位: University of Victoria
• 依托单位国家: 加拿大
• 项目类别: Discovery Grants Program - Accelerator Supplements
• 财政年份: 2008
• 资助国家: 加拿大
• 起止时间: 2008-01-01 至 2009-12-31
• 项目状态: 已结题
• 来源: https://www.nserc-crsng.gc.ca/ase-oro/Details-Detailles_eng.asp?id=401891
• 关键词: Probing; galaxies; quasar; absorption; lines

Distant quasars (also sometimes called QSOs) can be used as lighthouses at the edge of the universe to study galaxies that lie between them and the Earth. My research focuses on using the imprints of intervening galaxies on the spectra of quasars to study their formation and evolution. Whilst this technique is several decades old, my research is finding novel applications of the idea. For example, my team has perfected a technique for finding rare cases where the background QSO probes highly metal-enriched regions of an intervening galaxy. These sight lines are also expected to be rich in molecules which we can use to model the physical characteristics of the galaxy and even trace evolution of fundamental constants with time. In very extreme cases, we can even see the signatures of organic compounds and we have recently made the first detection of such features at cosmological distances.

遥远的类星体（有时也称为类星体）可以被用作宇宙边缘的灯塔，以研究位于它们和地球之间的星系。 我的研究重点是利用类星体光谱上的介入星系印记来研究它们的形成和演化。 虽然这种技术已经有几十年的历史了，但我的研究正在寻找这种想法的新应用。 例如，我的团队已经完善了一种技术，用于发现背景类星体探测居间星系中高度金属富集区域的罕见情况。 这些视线也有望富含分子，我们可以用它们来模拟星系的物理特性，甚至追踪基本常数随时间的演化。 在非常极端的情况下，我们甚至可以看到有机化合物的特征，我们最近首次在宇宙距离上检测到了此类特征。