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Galaxies and their Masks: A Conference in Honour of K.C. Freeman, FRS

机译:星系及其面具:纪念K.C.的会议弗里曼,FRS

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摘要

Various kinds of masks obscure our view of our galaxy, the Milky Way, as well as of other galaxies. Masks of interstellar dust affect our measurements within galaxies, on scales ranging from individual supernovae to the galaxies themselves. The “mass mask” (our inability to image mass rather than light) gives astronomers a very incomplete picture of the size and structure of galaxies themselves, because we cannot image the dark matter which provides most of the galactic mass. Another mass is the “dynamical mask”: as galaxies form, much dynamical information is lost in the birthing process. A new thrust in research is to retrieve such information by means of chemical tagging. About 50 astronomers flew into Namibia in April 2010, to celebrate the 70th birthday of Professor K.C. Freeman, Fellow of the Royal Society. At age 70, Freeman, a father of dark matter in galaxies, continues to be one of planet’s most highly cited astronomers. The current volume affords readers a unique perspective on galaxies by probing the thoughts of some of the greatest astronomers of our age. Contributions focus on galaxies from within our Local Group to those in our high redshift Universe. Approximately 40 in-depth review and contributed papers are contained in the volume, each written by an expert in the field. Two unusual features of the current volume include the “Star Country” of the San people of southern Africa as well as the introduction into astronomy of “The Treachery of Images” by the Belgian surrealist artist René Magritte. “Everything we see hides another thing, we always want to see what is hidden by what we see”, said Magritte. These words resonate the theme of the current volume “Galaxies and their Masks”, which is written at a level to be appreciated by both specialist and doctoral student alike.
机译:各种各样的面具使我们对银河系,银河系以及其他星系的视线模糊不清。星际尘埃的面具会影响我们在银河系中的测量,范围从单个超新星到银河系本身。 “质量掩膜”(我们无法像质而不是像质)无法为天文学家提供关于星系本身的大小和结构的非常不完整的图像,因为我们无法成像提供大部分银河质的暗物质。另一个质量是“动态蒙版”:随着星系的形成,在诞生过程中会丢失许多动态信息。研究的新方向是通过化学标记检索此类信息。为庆祝K.C.教授诞辰70周年,2010年4月,约50名天文学家飞往纳米比亚。弗里曼,皇家学会会员。弗里曼(Freeman)是星系暗物质之父,享年70岁,仍然是地球上被引用次数最多的天文学家之一。通过探究我们这个时代一些最伟大的天文学家的思想,本书为读者提供了关于星系的独特视角。贡献集中在本地组中的星系到高红移宇宙中的星系。该卷中包含约40篇深入的评论和贡献的论文,每篇论文均由该领域的专家撰写。当前卷的两个不寻常的特征包括南部非洲的桑人的“明星之乡”,以及比利时超现实主义艺术家勒内·马格里特(RenéMagritte)将“图像的背叛”引入天文学。马格里特说:“我们看到的一切都隐藏着另一件事,我们总是希望看到所看到的东西隐藏了什么。”这些词与当前的“银河及其面具”一书的主题产生共鸣,该书的写作水平受到专家和博士生的一致好评。

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