X-Ray Astronomy Study with the Astro-D Satellite

使用 Astro-D 卫星进行 X 射线天文学研究

• 批准号: 04044167
• 负责人: NAGASE Fumiaki
• 金额: $ 7.42万
• 依托单位: The Institute of Space and Astronautical Science
• 依托单位国家: 日本
• 项目类别: Grant-in-Aid for international Scientific Research
• 财政年份: 1992
• 资助国家: 日本
• 起止时间: 1992 至 1994
• 项目状态: 已结题
• 来源: https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-04044167/
• 关键词: X-ray astronomy; scientific satellite; X-ray spectroscopy; cosmic hot plasmas; X-ray sources; black holes; evolution of the universe; 軌道天文台; 超新星; 銀河団; 宇宙X線背景放射; X線望遠鏡; X線撮像; X線分光; X線CCD

ASCA (ASTRO-D), the fourth X-ray astronomy satellite of ISAS,was successfully launched on February 20,1993. It carries nested thin-foil X-ray mirrors providing a large effective area over a wide energy range from 0.5 to 10keV.A set of CCD cameras and imaging gas scintillation proportional counters are placed on the focal plane. ASCA is a high-throughput imaging and spectroscopic X-ray observatory with these instruments.An extensive collaboration between Japanese and U.S.scientists has been carried out in the joint developments of the X-ray telescopes, the X-ray CCD cameras, and computer software. It is continuing in the maintenance and the in-flight calibration of the instruments, and also in the data analysis and the following scientific activities.ASCA is an X-ray astronomy observatory which is, for the first time, capable of performing imaging and spectroscopic observations simultaneously over a wide energy range 0.5-10keV.The ASCA instruments cover the most important energy band for plasma diagnostics, because all the K-lines and the K-absorption edges from oxygen through iron at various ionization stages lie within this band. The CCD camera of ASCA can resolve all major lines individually. Motion of plasma of the order or greater than 1000km/s can be measured significantly from Doppler shift of the line energies. These capabilities of ASCA allow diagnostics of accreting matter around such compact objects as neutron stars and black holes. Spatially-resolved spectroscopy with ASCA also provides powerful means for the investigations of extended plasmas in supernova remnants, galaxies, and clusters of galaxies.The key elements of ASCA are succesfully working in orbit. ASCA has already obtained several remarkable scientific results. Most of them are due to the Japan-US collaboration with the help of this International Scientific Research Program as A Grant-in Aid for Scientific Research.

ASCA（ASTRO-D）是ISAS的第四颗X射线天文卫星，于1993年2月20日成功发射。它携带嵌套的薄箔X射线反射镜，在0.5至10 keV的宽能量范围内提供大的有效面积。一组CCD相机和成像气体闪烁正比计数器被放置在焦平面上。ASCA是一个高通量成像和光谱X射线天文台，拥有这些仪器。日本和美国科学家在X射线望远镜、X射线CCD相机和计算机软件的联合开发方面进行了广泛的合作。它继续进行仪器的维护和飞行中校准，以及数据分析和后续科学活动。ASCA是一个X射线天文观测台，首次能够在0.5- 10 keV的宽能量范围内同时进行成像和光谱观测。ASCA仪器覆盖了等离子体诊断最重要的能带，因为所有的K线和在不同电离阶段从氧到铁的K吸收边都在这个带内。ASCA的CCD相机可以单独解析所有主要线条。从谱线能量的多普勒频移可以很好地测量出等离子体的速度在1000 km/s量级或以上的运动。ASCA的这些能力允许诊断中子星和黑洞等致密物体周围的吸积物质。ASCA的空间分辨光谱学也为超新星遗迹、星系和星系团中扩展等离子体的研究提供了强有力的手段。ASCA已经取得了一些显著的科学成果。其中大部分是由于日本和美国的合作，在这个国际科学研究计划的帮助下，作为一个赠款援助科学研究。

项目成果

槙野 文命ほか: "“New Horizon of X-Ray Astronomy"集録" ユニバーサル アカデミー プレス, 700

Fumi Makino 等人：““X 射线天文学的新视野”收藏”Universal Academy Press，700

Y.Tanaka: "Black Hole X-Ray Binaries" Proceedings of the Ginga Memorial Symposium (ISAS Symposium on Astrophysics 1992). 19-36 (1992)

Y.Tanaka：“黑洞 X 射线双星”Ginga 纪念研讨会论文集（ISAS 天体物理学研讨会 1992）。

R.Mushotzky,and BBXRT Team: "BBXRT Observations and Their Relevance for ASTRO-D" Proceedings of the Ginga Memorial Symposium (ISAS Symposium on Astrophysics 1992). 139-148 (1992)

R.Mushotzky 和 ​​BBXRT 团队：“BBXRT 观测及其与 ASTRO-D 的相关性”Ginga 纪念研讨会论文集（ISAS 天体物理学研讨会 1992）。

P.Serlemitsos et al.: "The Complex X-ray Spectra of Two High Redshift-Quasars Observed with ASCA" Publ.Astron.Soc.Japan. 46. L43-L47 (1994)

P.Serlemitsos 等人：“用 ASCA 观测到的两个高红移类星体的复杂 X 射线光谱”Publ.Astron.Soc.Japan。

S.S.Holt.et al.: "ASCA Obsservations of Cassiopeia A" Publ.Astron.Soc.Japan. 46. L151-L155 (1994)

S.S.Holt.等人：“ASCA 对仙后座 A 的观测”Publ.Astron.Soc.Japan。