Galactic and Extragalactic Research with Schmidt Telescopes

这项拨款支持彼得佩施和尼古拉斯博士的研究 Sanduleak基于对凯斯西储的观察 位于年基特峰的伯勒尔施密特望远镜 亚利桑那州，并与柯蒂斯施密特，位于塞罗托洛洛 美洲天文台。 现在的主要调查是 进行的是一个非常富有成效的搜索幽蓝和/或 发射线星系，准恒星物体， 发射特征，可能的蓝色恒星，主序星晚B和 A型星，星族II型星A型和F型，F型和G型次矮星， 暗碳星和晚M型星。 探索性观察 在Burrell施密特上安装电荷耦合装置 以确定直接和光谱观测 这些计划值得去做。 银河系结构和星系分布的研究 河外天体需要巡天来识别 对此将进行详细研究。 对大部分地区的调查 天空对于研究人口特别重要 分布来确定不同的 向核、晕、反中心方向的特征。 的 凯斯西方的这些研究人员进行的调查是 这是进行详细后续调查的重要第一步。

This grant supports research by Drs. Peter Pesch and Nicholas Sanduleak based on observations made with Case Western Reserve University's Burrell Schmidt telescope, located on Kitt Peak in Arizona, and with the Curtis Schmidt, located at Cerro Tololo Inter-American Observatory. The principal survey now being carried out is a very fruitful search for faint blue and/or emission line galaxies, quasi-stellar objects with and without emission features, probable blue stars, main-sequence late B and A stars, Population II stars of types A and F, F and G subdwarfs, and faint carbon and late M type stars. Exploratory observations with a charge coupled device on the Burrell Schmidt are planned to determine what direct and spectroscopic observational programs would be worthwhile to undertake. Investigations of galactic structure and the distribution of extragalactic objects require surveys to identify the objects which will be studied in detail. Surveys over large parts of the sky are especially important for studies of the population distribution in our galaxy to determine the different characteristics towards the nucleus, halo and anticenter. The surveys conducted by these researchers at Case Western are a vital first step to detailed follow-on investigations.