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Arnab Sarkar

massachusetts institute of technology
H指数:12
被引数:567

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Metallicity Gradients in Modern Cosmological Simulations. II. The Role of Bursty versus Smooth Feedback at High Redshift

金属丰度梯度在现代宇宙学模拟中的作用。II. 高红移下爆发式与平滑反馈的作用

2026-04-160
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
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
Cold Gas and Star Formation in the Phoenix Cluster with JWST

凤凰星系团中的冷气体与恒星形成(JWST)

2025-08-120
PRE
Metallicity Gradients in Modern Cosmological Simulations. I. Tension between Smooth Stellar Feedback Models and Observations

宇宙学模拟中的金属丰度梯度。I. 平滑恒星反馈模型与观测之间的紧张关系

2025-08-110
PRE
Cataclysmic Variables and AM CVn Binaries in SRG/eROSITA plus Gaia: Volume Limited Samples, X-Ray Luminosity Functions, and Space Densities
2025-01-091
OA
Mapping the Imprints of Stellar and Active Galactic Nucleus Feedback in the Circumgalactic Medium with X-Ray Microcalorimeters
2024-07-030
OA
Mapping the intracluster medium in the era of high-resolution X-ray spectroscopy
2024-04-176
OA