首页> 外文期刊>The Astrophysical Journal. Supplement Series >X-Atlas: An Online Archive of Chandra's Stellar High-Energy Transmission Grating Observations
【24h】

X-Atlas: An Online Archive of Chandra's Stellar High-Energy Transmission Grating Observations

机译:X-Atlas:钱德拉的恒星高能透射光栅观测结果在线存档

获取原文
获取原文并翻译 | 示例
       

摘要

The high-resolution X-ray spectroscopy made possible by the 1999 deployment of the Chandra X-ray Observatory has revolutionized our understanding of stellar X-ray emission. Many puzzles remain, however, particularly regarding the mechanisms of X-ray emission from OB stars. Although numerous individual stars have been observed in high resolution, realizing the full scientific potential of these observations will necessitate studying the high-resolution Chandra data set as a whole. To facilitate the rapid comparison and characterization of stellar spectra, we have compiled a uniformly processed database of all stars observed with the Chandra High-Energy Transmission Grating (HETG). This database, known as X-Atlas, is accessible through a Web interface with searching, data retrieval, and interactive plotting capabilities. For each target, X-Atlas also features predictions of the low-resolution ACIS spectra convolved from the HETG data for comparison with stellar sources in archival ACIS images. Preliminary analyses of the hardness ratios, quantiles, and spectral fits derived from the predicted ACIS spectra reveal systematic differences between the high- and low-mass stars in the atlas and offer evidence for at least two distinct classes of high-mass stars. A high degree of X-ray variability is also seen in both high- and low-mass stars, including Capella, long thought to exhibit minimal variability. X-Atlas contains over 130 observations of approximately 25 high-mass stars and 40 low-mass stars and will be updated as additional stellar HETG observations become public. The atlas has recently expanded to nonstellar point sources, and Low-Energy Transmission Grating (LETG) observations are currently being added as well.
机译:钱德拉X射线天文台1999年的部署使高分辨率X射线光谱学成为可能,彻底改变了我们对恒星X射线发射的理解。但是,仍然存在许多困惑,特别是关于OB星发出X射线的机制。尽管已经以高分辨率观察到许多独立的恒星,但要实现这些观察的全部科学潜力,就必须对整个高分辨率Chandra数据集进行整体研究。为了便于快速比较和表征恒星光谱,我们已经编译了使用钱德拉高能透射光栅(HETG)观测到的所有恒星的统一处理数据库。该数据库称为X-Atlas,可通过具有搜索,数据检索和交互式绘图功能的Web界面进行访问。对于每个目标,X-Atlas还具有根据HETG数据对低分辨率ACIS光谱进行预测的功能,以便与档案ACIS图像中的恒星源进行比较。从预测的ACIS光谱得出的硬度比,分位数和光谱拟合的初步分析揭示了地图集中高质量恒星和低质量恒星之间的系统差异,并为至少两种不同类别的高质量恒星提供了证据。长期以来,包括卡佩拉(Capella)在内的高质量和低质量恒星中都发现了高度的X射线变异性,长期以来人们一直认为它们表现出最小的变异性。 X-Atlas包含大约25个高质量恒星和40个低质量恒星的130多个观测值,并将随着其他恒星HETG观测值的公开而更新。该地图集最近已扩展到非恒星点源,并且目前也正在添加低能透射光栅(LETG)观测资料。

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