The Mass Distribution and Evolution of Galaxy Groups

AST-0506628 Wilcots绝大多数星系，包括银河系，都存在于称为星系群的松散集合中，这意味着如果不考虑星系群的作用，就无法彻底了解星系的演化。 迄今为止，X射线和光学研究似乎表明，星系团的物理特征与较大星系团的物理特征有很大的差异。 由螺旋星系主导的星系群与由椭圆星系主导的星系群有很大的不同。 这项对低红移和中等红移星系群的广泛观测研究旨在解决两个基本问题：星系群中质量的真实分布是什么，以及星系群如何随时间演化？ 主要（无线电）观测将包括一次HI调查、一次深连续谱调查、一次弯曲射电源研究和一次绘制弥散连续谱发射图的试验性实验。 更广泛的影响集中在公共宣传的公园宇宙计划，本科生参与研究，并继续致力于吸引代表性不足的少数民族。

AST-0506628WilcotsThe vast majority of galaxies, including the Milky Way, reside in loose collections called groups, which means that a thorough understanding of galaxy evolution cannot be achieved without considering the role of groups. X-ray and optical studies so far seem to show that the physical characteristics of groups deviate significantly from those of larger clusters. Groups dominated by spiral galaxies differ dramatically from groups dominated by ellipticals. This broad observational study of galaxy groups at low and intermediate redshift is designed to address two fundamental questions: what is the true distribution of mass in groups, and how have groups evolved over time? The principal (radio) observations will include an HI survey, a deep continuum survey, a study of bent radio sources, and a pilot experiment to map the diffuse continuum emission. Complementary optical observations will also be brought to bear on this study.Broader impacts center on the Universe in the Park program of public outreach, involvement of undergraduate students in the research, and a continued commitment to attracting underrepresented minorities.