首页     开始     To Survive in the Universe    
Inhabited Sky
    News@Sky     天文图片     收集     论坛     Blog New!     常见问题     新闻     登录  

HD 187741


目录

图像

上传图像

DSS Images   Other Images


相关文章

The structure of the interstellar gas towards stars in the globular cluster M 55
Observations are presented of high resolution interstellar Na D lineprofiles towards 10 stars in the globular cluster M 55 and 6 foregroundstars which lie within 3 deg from the cluster. The spectral regioncontaining the K I (lambda 7699 A) line is simultaneously recorded butthis line is detected only towards one of the foreground stars as acomponent having a relatively high K I/Na I abundance ratio. Twoprincipal components are observed towards the cluster stars atvelocities of approximately +1 and +15 km/s and weaker higher velocitygas is detected at approximately -21, +33 and +55 km/s. The +1 km/scomponent is at a distance of approximately less than 100 pc and wesuggest that this is part of an extensive region of diffuse gas whichconnects the molecular and dark clouds observed closer to the galacticplane. The +15 km/s component lies at a distance between 130 to 300 pcand is identified with an anomalous velocity arc observed in HI. Thehigher velocity gas components are at a distance approximately greaterthan 700 pc. From a comparison with our previous observations in thegeneral direction of the Carina-Sagittarius arm we suggest that thesefeatures have an origin in spiral arm gas, in which case their detectiontowards M 55 places them some 600 to 800 pc from the galactic plane.

提交文章


相关链接

  • - 没有找到链接 -
提交链接


下列团体成员


观测天体数据

星座:人馬座
右阿森松:19h52m44.34s
赤纬:-31°58'36.3"
视星:7.106
距离:1176.471 天文距离
右阿森松适当运动:2.7
赤纬适当运动:-6.8
B-T magnitude:7.319
V-T magnitude:7.124

目录:
适当名称   (Edit)
HD 1989HD 187741
TYCHO-2 2000TYC 7443-1623-1
USNO-A2.0USNO-A2 0525-41690812
HIPHIP 97824

→ 要求更多目录从vizier