XMM-Newton observations of ζ Puppis
收藏arXiv2011-12-05 更新2024-08-06 收录
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http://arxiv.org/abs/1112.0862v1
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资源简介:
本数据集由列日大学和Guanajuato大学合作,通过XMM-Newton卫星对ζ Puppis星进行了18次观测,总曝光时间达到1Ms。数据集包含高分辨率X射线光谱,用于研究该星的X射线辐射特性及其随时间的变化。ζ Puppis是一颗距离地球仅335光年的明亮大质量星,其X射线辐射稳定,但光谱线形随波长变化。此数据集有助于深入理解大质量星的X射线辐射机制及其与星风的相互作用,为解决星体物理中的关键问题提供了重要数据支持。
This dataset was developed in collaboration between the University of Liège and the University of Guanajuato, which conducted 18 observations of the ζ Puppis star using the XMM-Newton satellite, with a total exposure time of 1 Ms. The dataset contains high-resolution X-ray spectra for studying the X-ray emission properties of this star and its temporal variability. ζ Puppis is a bright massive star located just 335 light-years from Earth, with stable X-ray emission but its spectral line profiles varying with wavelength. This dataset facilitates in-depth understanding of the X-ray emission mechanisms of massive stars and their interactions with stellar winds, providing critical data support for resolving key issues in stellar physics.
提供机构:
列日大学
创建时间:
2011-12-05



