Showing 41–60 of 67 results
/ Date/ Name
Sep 4, 2025Disentangling Multiple Gas Kinematic Drivers in the Perseus Galaxy ClusterOct 7, 2025Comparing XRISM cluster velocity dispersions with predictions from cosmological simulations: are feedback models too ejective?Jun 5, 2025Unraveling the structure of the stratified ultra-fast outflows in PDS 456 with XRISMDec 10, 2025Delving into the depths of NGC 3783 with XRISM IV. Mapping of the accretion flow with Fe K$α$ emission linesFeb 22, 2023X-ray time lag evaluation of MAXI J1820+070 with a differential cross-correlation analysisOct 21, 2022A novel "spectral-ratio model fitting" to resolve complicated AGN X-ray spectral variationsMar 6, 2019FeI lines in 0.91-1.33 ${\rm μ}$m spectra of red giants for measuring the microturbulence and metallicitiesFeb 22, 2016Near infrared diffuse interstellar bands toward the Cygnus OB2 associationOct 20, 2025Discovery of Powerful Multi-Velocity Ultra-Fast Outflows in the Starburst Merger Galaxy IRAS 05189$-$2524 with XRISMSep 18, 2025First Detection of X-ray Polarization and Its Short-term Increase Pre- and Post-Eclipse in HMXB 4U 1700-377Aug 19, 2025In orbit operation of Resolve Filter Wheel and MXSJul 2, 2025XRISM analysis of the complex Fe K$α$ line in Centaurus AApr 29, 2025XRISM forecast for the Coma cluster: stormy, with a steep power spectrumDec 9, 2025Delving into the depths of NGC 3783 with XRISM III. Birth of an ultrafast outflow during a soft flareApr 8, 2026Complex Nuclear Structure in Seyfert 2 Galaxy NGC 4388 Revealed by XRISM ObservationFeb 18, 2026Resolving the Multiple Component Outflows in PG 1211+143: II. The Soft X-ray View of the Ultra Fast OutflowOct 20, 2020Mg II and Fe II fluxes of luminous quasars at z ~ 2.7 and evaluation of the Baldwin effect in the flux-to-abundance conversion method for quasarsMar 14, 2024[N I] 10400/10410 Å Lines as Possible Disk Wind Tracers in a Young Intermediate-Mass StarMar 14, 2023A broadband X-ray imaging spectroscopy in the 2030s: the FORCE missionNov 30, 2021Warm Absorbers in the Radiation-driven Fountain Model of Low-mass Active Galactic Nuclei