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星系团Abell 2199的恒星形成性质
  • ISSN号：0001-5245
  • 期刊名称：《天文学报》
  • 时间：0
  • 分类：P157.8[天文地球—天文学]
  • 作者机构：[1]南京师范大学物理科学与技术学院,南京,210097 南京师范大学物理科学与技术学院,南京,210097 江苏工业学院信息科学系,常州,213164 南京师范大学物理科学与技术学院,南京,210097 南京信息职业技术学院微电子系,南京,210046
  • 相关基金：国家自然科学基金项目(10778618,10633020)
作者： 袁启荣[1], 何莹莹[1], 李峰[1], 张立[1], 赵丽芳[1]
关键词： 星系, 星系团, 个别, 星系, 基本参数, 星系, 运动学与动力学
中文摘要：

通过对近邻星系团Abell 2199中290颗成员星系进行形态分类,研究这些星系的恒星形成率及其与形态和相关物理特性之间的关系.该星系团中星系的特征恒星形成率与Ha等值宽度、星系光谱在4000A处的跃变程度以及星系所包含的恒星质量之间有较强的相关性.这些星系的恒星形成活动没有表现出明显的环境效应,表明该星系团仍处在剧烈的动力学演化阶段,远没有达到动力学平衡.

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近邻星系团动力学及其成员星系的恒星形成性质
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期刊信息
  • 《天文学报》
  • 中国科技核心期刊
  • 主管单位:中国科学院
  • 主办单位:中国天文学会 中国科学院紫金山天文台
  • 主编：甘为群
  • 地址：南京市栖霞区元化路8号
  • 邮编：210023
  • 邮箱：twxb@pmo.ac.cn
  • 电话：025-83332133
  • 国际标准刊号：ISSN：0001-5245
  • 国内统一刊号：ISSN：32-1113/P
  • 邮发代号:2-818
  • 获奖情况:
  • 1992年获中国科协优秀期刊三等奖,1996年获中国科学院优秀期刊三等奖,2000年获中国科协优秀期刊三等奖,中国期刊方阵“双效”期刊
  • 国内外数据库收录:
  • 日本日本科学技术振兴机构数据库,中国中国科技核心期刊,中国北大核心期刊（2004版）,中国北大核心期刊（2008版）,中国北大核心期刊（2011版）,中国北大核心期刊（2014版）,中国北大核心期刊（2000版）
  • 被引量:1792