首页> 外文期刊>The Astrophysical journal >The Solar Neighborhood. XV. Discovery of New High Proper Motion Stars with μ ≥ 04 yr?1 between Declinations ?47° and 00°
【24h】

The Solar Neighborhood. XV. Discovery of New High Proper Motion Stars with μ ≥ 04 yr?1 between Declinations ?47° and 00°

机译:太阳街区。十五在偏角?47°和00°之间发现μ≥04 yr?1的新的高适速运动恒星

获取原文
           

摘要

We report the discovery of 152 new high proper motion systems (μ ≥ 04 yr-1) in the southern sky (δ = -47° to 00°) brighter than UKST plate R59F = 16.5 via our SuperCOSMOS-RECONS (SCR) search. This paper complements Paper XII in the Solar Neighborhood series, which covered the region from δ = -90° to -47° and discussed all 147 new systems from the southernmost phase of the search. Among the total of 299 systems from both papers, there are 148 (71 in Paper XII, 77 in this paper) new systems moving faster than 05 yr-1 that are additions to the classic Luyten Half Second sample. These constitute an 8% increase in the sample of all stellar systems with μ ≥ 05 yr-1 in the southern sky. As in Paper XII, distance estimates are provided for the systems reported here based on a combination of photographic plate magnitudes and Two Micron All Sky Survey photometry, assuming that all stars are on the main sequence. Two SCR systems from the portion of the sky included in this paper are anticipated to be within 10 pc, and an additional 23 are within 25 pc. In total, the results presented in Paper XII and here for this SCR sweep of the entire southern sky include five new systems within 10 pc and 38 more between 10 and 25 pc. The largest number of nearby systems have been found in the slowest proper motion bin, 06 yr-1 > μ ≥ 04 yr-1, indicating that there may be a large population of low proper motion systems very near the Sun.
机译:通过我们的SuperCOSMOS-RECONS(SCR)搜索,我们报告发现在南部天空(δ= -47°至00°)中比UKST板R59F = 16.5亮的152个新的高适当运动系统(μ≥04 yr-1)。本文是“太阳邻里”系列论文XII的补充,后者涵盖了δ= -90°到-47°的区域,并讨论了搜索最南端的所有147个新系统。在这两篇论文的总共299个系统中,有148个(比第十二论文中的71个,本文中的77个)新系统的运行速度快于05 yr-1,这是经典Luyten Half Second样本的补充。在南部天空中,μ≥05 yr-1的所有恒星系统的样本中,这些值增加了8%。与论文XII中一样,此处假设的所有星基都在主序列上,这是基于照相板幅值和两微米全天候光度学测光法的结合为此处报告的系统提供距离估计的。本文中包括的两个SCR系统预计在10 pc以内,另外23个SCR系统在25 pc以内。总体而言,论文XII和此处针对整个南部天空的SCR扫描所显示的结果包括10个pc内的五个新系统,以及10到25 pc之间的38个新系统。在最慢的固有运动仓中发现了最多的附近系统,即06 yr-1>μ≥04 yr-1,这表明在太阳附近可能存在大量的低固有运动系统。

著录项

获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号