...
首页> 外文期刊>The Astrophysical journal >FAR ULTRAVIOLET SPECTROSCOPIC EXPLORER OBSERVATIONS OF THE ACTIVE COOL STAR AB DORADUS
【24h】

FAR ULTRAVIOLET SPECTROSCOPIC EXPLORER OBSERVATIONS OF THE ACTIVE COOL STAR AB DORADUS

机译:活性COOL STAR AB DORADUS的远紫外光谱探索者观察

获取原文
获取原文并翻译 | 示例

摘要

Far-ultraviolet spectra were obtained of the active cool star AB Doradus (HD 36705) during the calibration and checkout period of the Far Ultraviolet Spectroscopic Explorer (FUSE) satellite. Observations in this early phase of the mission were taken at a resolving power of 12,000-15,000 (~20-25 km s~(-1)) and covered the spectral range 905-1187 A. The integrated spectrum exhibits strong, rotationally broadened stellar emission from C Ⅲ (λλ977, 1175) and O Ⅵ (λλ1032, 1037) and many weaker lines. Strong emission lines of C Ⅲ and O Ⅵ exhibit broad wings. The C Ⅲ λ977 profile shows blueshifted absorption at ~30 km s~(-1), and C Ⅱ λ1036 absorption appears superposed on emission in the wing of O Ⅵ λ1037. Rotational modulation of C Ⅲ and O Ⅵ is present, in harmony with its photometric variability. Flares were detected in the brightest lines, and subexposures were analyzed to examine flux and profile variations. Downflows that extend to 600 km s~(-1) during a flare are found in the O Ⅵ profiles. These early observations demonstrate that FUSE will be an exceptional instrument for studying chromospheres in cool stars.
机译:在“远紫外光谱浏览器”(FUSE)卫星的校准和检验期间,获得了活跃的冷星AB Doradus(HD 36705)的远紫外光谱。任务早期阶段的观测是在12,000-15,000(〜20-25 km s〜(-1))的分辨力下进行的,覆盖了905-1187 A的光谱范围。合并后的光谱显示出强的,旋转加宽的恒星CⅢ(λλ977,1175)和OⅥ(λλ1032,1037)和许多较弱的谱线发射。 CⅢ和OⅥ的强发射线展宽。 CⅢλ977剖面在〜30 km s〜(-1)处出现蓝移吸收,CⅡλ1036吸收出现在OⅥλ1037机翼的发射上。存在CⅢ和OⅥ的旋转调制,与其光度变异性相一致。在最亮的线条中检测到耀斑,并对次曝光进行分析以检查通量和轮廓变化。在OⅥ剖面中发现了在爆发过程中延伸到600 km s〜(-1)的下流。这些早期的观察结果表明,FUSE将是研究凉爽恒星中色球的一种特殊工具。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
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