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20242026
most citedSpectral and photometric variability of SS 433 observed with XRISM and simultaneous optical and near-infrared telescopes

3 citations · 4 across the 4 of their papers we have counts for

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astro-ph.HE2026

Tracing the Orbital Motion of the Accreting White Dwarf in EX~Hydrae with XRISM/Resolve

Yuken Ohshiro, Yukikatsu Terada, Taichi Ichikawa +7

Measuring the masses of accreting white dwarfs (WDs) is crucial for understanding their evolution and the physics of accretion. High-resolution X-ray spectroscopy can trace the WD…

astro-ph.HE20261 cited

Plasma Dynamics of Radiative Cooling Accretion Flow in AM Herculis with XRISM

Yukikatsu Terada, Kaya Mori, Takayuki Hayashi +14

We present XRISM/Resolve high-resolution X-ray spectroscopy of the prototypical magnetic cataclysmic variable AM Herculis. All satellite lines of highly ionized Fe are fully resolv…

astro-ph.HE2026

Disk instability model incorporating a variable inner disk radius in SS Cyg and U Gem

Mariko Kimura, Osaki Yoji

Previous theoretical studies indicate that the inner disk in dwarf novae evaporates into a high-temperature, optically thin, and geometrically thick accretion flow during quiescenc…

astro-ph.HE20263 cited

Spectral and photometric variability of SS 433 observed with XRISM and simultaneous optical and near-infrared telescopes

Yusuke Sakai, Shinya Yamada, Yuta Okada +36

We present results from coordinated multiwavelength observations of the SS 433, obtained with XRISM, optical telescopes, and near-infrared camera during 2024 April and 2025 March.…

astro-ph.HE2025

Evolution of the inner accretion flow and the white-dwarf spin pulse during the 2023 outburst in GK Persei

Mariko Kimura, Takayuki Hayashi, Yuuki Wada +8

We present our X-ray and optical observations performed by NICER, NuSTAR, and Tomo-e Gozen during the 2023 outburst in the intermediate polar GK Persei. The X-ray spectrum consiste…

astro-ph.HE2024

Evolution of X-ray and optical rapid variability during the low/hard state in the 2018 outburst of MAXI J1820+070 = ASASSN-18ey

Mariko Kimura, Hitoshi Negoro, Shinya Yamada +3

We performed shot analyses of X-ray and optical sub-second flares observed during the low/hard state of the 2018 outburst in MAXI J1820070. Optical shots were less spread than X…