王裔龙
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I study the accretion of compact objects with a particular focus on X-ray binaries. My work combines theoretical modeling of accretion flows with observational studies of Galactic X-ray transients using data from missions such as Einstein Probe. Through this combination of theory and observation, I aim to clarify how matter accretes under extreme conditions.
2026.9 - Present: Postdoctoral researcher
Institute of Space Sciences (ICE, CSIC), Barcelona, Spain
2021.9 - 2026.6: PhD in Astrophysics, supervised by Prof. Bifang Liu
National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China
2025.2 - 2026.2: visiting PhD student, supervised by Prof. Nanda Rea Institute of Space Sciences (ICE, CSIC), Barcelona, Spain
2017.9 - 2021.6: BSc in Astronomy, supervised by Prof. Bifang Liu
University of Chinese Academy of Sciences, Beijing, China
2023.7 - Present: associate member of the Einstein Probe Science Topical Panel 4 (compact stellar objects)
2024.1 - Present: transient advocate of the Einstein Probe
2022.9 - 2025.2: transient advocate of the Lobster Eye Imager for Astronomy (LEIA)
2022.9 - 2026.3: teaching assistant of the postgraduate course Radiative Processes in Astrophysics at the University of Chinese Academy of Sciences
[1] Wang Y L, et al., 2026. Einstein Probe discovery of EP J171159.4-333253: an eclipsing neutron star low-mass X-ray binary with clocked bursts. ApJ, 1003, 22.
[2] Wang Y L, et al., 2025. Accretion with two-phase gas supply and its application in black hole X-ray binaries. MNRAS, 544(2): 1833-1842.
[3] Wang Y L, et al., 2024. Accretion flows in the hard state of black hole X-ray binaries: the effect of hot gas condensation. MNRAS, 527(1): 1333-1343.
[4] Meyer-Hofmeister E, Wang Y L, et al., 2026. Accretion geometry in neutron star low-mass X-ray binaries during the hard spectral state. MNRAS, 545(4): 1-8.
[5] Imbrogno M, Veresvarska M, Wang Y L, et al., 2026. The X-ray emission of the long-period transient and accreting cataclysmic variable ASKAP J174508.9-505149. A&A, 710, L27.
[6] Coti Zelati F, Marino A, Wang Y L, et al., 2026. Multi-wavelength Outburst Activity from EP J174942.2-384834: a very faint X-ray transient discovered by Einstein Probe. ApJ, 1003, 224.
[7] Liu M, Liu B F, Wang Y L, et al., 2025a. A generalized solution for advection-dominated accretion flow, standard disc and slim disc. MNRAS, 539(1): 69-81.
[8] Liu M, Liu B F, Wang Y L, et al., 2025b. The effectively optically thin accretion flow and its implication in supermassive black holes. MNRAS, 541(2): 1231-1240.
[9] Rose K, et al., 2026. Periodic Radio and X-ray Emission from an Accreting White Dwarf Binary. Nat. Astron. accepted
[10] Sun H, et al., 2025. A fast X-ray transient from a weak relativistic jet associated with a type Ic-BL supernova. Nat. Astron., 9: 1073-1085.
[11] Liu Y, et al., 2025. Soft X-ray prompt emission from the high-redshift gamma-ray burst EP240315a. Nat. Astron., 9: 564-576.
[12] Zhang W, et al., 2025. Einstein Probe discovery of EP240408a: A peculiar X-ray transient with an intermediate timescale. SCPMA, 68(1), 219511: 219511.
[13] Li D, et al., 2026. A fast powerful X-ray transient from possible tidal disruption of a white dwarf. Sci. Bull., 71(3): 538-546.
[14] Marino A, et al., 2026. Aql X-1 from dawn ’til dusk: the early rise, fast state transition and decay of its 2024 outburst. A&A, 710, A115.
[15] Ling Z X, et al., 2023. The Lobster Eye Imager for Astronomy Onboard the SATech-01 Satellite. RAA, 23(9), 095007: 095007.
