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Hiroyuki Uchida

kyoto university
H指数:22
被引数:1,939

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Origin of the Stellar Fe Kα Line Clarified with Far-ultraviolet and X-Ray Observations of a Superflare on the RS Canum Venaticorum-type Star UX Arietis

通过RS Canum Venaticorum型恒星UX Arietis的超耀斑的远紫外和X射线观测澄清恒星Fe Kα线的起源

2026-05-010
PRE
Asymmetric Distribution of Fe-peak Elements in Cassiopeia A Revealed by XRISM

仙后座A中Fe-peak元素的分布不对称性由XRISM揭示

2026-04-030
OAAI
A XRISM/Resolve View of the Dynamics in the Hot Gaseous Atmosphere of M87

XRISM/Resolve对M87热气体大气层中动力学特征的观测视角

2026-02-110
OAAI
XRISM Constraints on Unidentified X-Ray Emission Lines; Including the 3.5 keV Line; in the Stacked Spectrum of 10 Galaxy Clusters

XRISM对10个星系团堆叠光谱中未识别X射线发射线(包括3.5 keV线)的限制;

2025-11-180
OA
XRISM/Resolve view of Abell 2319: Turbulence, sloshing, and ICM dynamics

阿贝尔2319的XRISM/Resolve视图: 湍流、晃动和ICM动力学

2025-11-013
PRE
Comparing XRISM Cluster Velocity Dispersions with Predictions from Cosmological Simulations: Are Feedback Models Too Ejective?

将XRISM星系团速度弥散度与宇宙学模拟预测进行比较:反馈模型是否过于喷射性?

2025-10-240
OA
Kinematic Evidence for Bipolar Ejecta Flows in the Galactic Supernova Remnant W49B

银河系超新星遗迹W49B中双极抛射流运动学证据

2025-07-280
PRE
XRISM Spectroscopy of the Fe Kα Emission Line in the Seyfert Active Galactic Nucleus NGC 4151 Reveals the Disk, Broad-line Region, and Torus
2024-09-190
OA
The XRISM/Resolve View of the Fe K Region of Cyg X-3

XRISM/Resolve对Cyg X-3 Fe K区域的观测结果

2024-01-010
OAAI