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arXiv 1102.4815astro-ph.SR
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亚毫米望远镜的自适应辐射转移创新(ARTIST)

Adaptable Radiative Transfer Innovations for Submillimeter Telescopes (ARTIST)

Marco Padovani, Jes Jørgensen

摘要:

亚毫米波观测是回答现代天体物理学中许多重大问题的关键,例如恒星和行星如何形成,星系如何演化,以及物质如何在恒星和星际介质中循环。随着ALMA和Herschel大型亚毫米波设备的建成,将为研究这些问题打开一扇新的窗口。ARTIST是欧洲ASTRONET计划资助的一个项目,目的是开发下一代模型套件,用于对尘埃和线发射及其偏振进行全面的多维辐射转移计算,以帮助解释这些突破性设施的观测结果。

英文摘要:

Submillimeter observations are a key for answering many of the big questions in modern-day astrophysics, such as how stars and planets form, how galaxies evolve, and how material cycles through stars and the interstellar medium. With the upcoming large submillimeter facilities ALMA and Herschel a new window will open to study these questions. ARTIST is a project funded in context of the European ASTRONET program with the aim of developing a next generation model suite for comprehensive multi-dimensional radiative transfer calculations of the dust and line emission, as well as their polarization, to help interpret observations with these groundbreaking facilities.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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