77 citations · 217 across the 8 of their papers we have counts for
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astro-ph.HE2024★ 1 cited
Examining the evolution of the Supersoft X-ray Source RX J0513.9-6951
A. Tavleev, V. F. Suleimanov, K. Werner +1
Supersoft X-ray sources (SSS) are thought to be accreting white dwarfs (WDs) in close binary systems, with thermonuclear burning on their surfaces. The SSS RX J0513.9-6951 in the L…
astro-ph.HE2024★ 2 cited
Soft X-ray emission from the classical nova AT 2018bej
A. Tavleev, L. Ducci, V. F. Suleimanov +4
Classical novae are known to demonstrate a supersoft X-ray source (SSS) state following outbursts, which is associated with residual thermonuclear burning on the white dwarf (WD) s…