标题： 恒星爆发星系的紫外到亚毫米SED建模 显示英文标题

标题： Modelling the UV to sub-mm SED of Starburst Galaxies

摘要： 本文综述了星暴星系的理论建模，特别强调了气相物理在决定连续谱SED形式和发射线光谱方面的重要性。 发射线和连续谱诊断都被用作恒星形成指标。 在这里，我们从理论的角度考察这些指标的可靠性以及它们对星系物理的敏感性，目的是减少与测量宇宙恒星形成历史相关的误差。 显示英文摘要

摘要： This paper reviews the theoretical modelling of starburst galaxies with particular emphasis on the importance of the gas-phase physics in determining the form of the continuum SED and the emission line spectrum. Both line and continuum diagnostics have been used as star formation indicators. Here, we examine from the point of view of the theory how reliable each of these indicators may be, and to what physics of the galaxy they are sensitive, with the aim of decreasing the errors associated with measuring the star formation history of the universe.