collaborators

9 papers

astro-ph.HE2026

Early Near-Infrared Excess and Rapid Disk-Corona Evolution in the Tidal Disruption Event 2024aepd

Yongxin Wu, Yanan Wang, Thomas M. Reynolds +38

The paper reports multi-wavelength observations of tidal disruption event 2024aepd, revealing an early near‑infrared excess and a rapid transition from a thermal X‑ray disk to a ha…

astro-ph.HE2026

Bolometric correction factor and radiative efficiency for the super-Eddington accretion flow in tidal disruption events

Yongxin Wu, Erlin Qiao, Xuan Fang +3

The estimate of the bolometric luminosity and the radiative efficiency are two key aspects for understanding the properties of the accretion flow around a supermassive black hole (…

astro-ph.SR2025

A Morpho-kinematic Study of Galactic High-ADF PNe Based on the VLT/UVES Deep Spectroscopy

Haomiao Huang, Xuan Fang, Jorge Garcia-Rojas +3

We report detailed analyses of deep, high-resolution spectra of three Galactic planetary nebulae (PNe) with high abundance discrepancy factors (ADFs), Hf2-2, M1-42 and NGC6153, obt…

astro-ph.SR2025

PyEMILI: A New Generation Computer-aided Spectral Line Identifier -- II. Emission-line Identification and Plasma Diagnostics of a Sample of Gaseous Nebulae

Zhijun Tu, Xuan Fang, Jorge García-Rojas +2

In order to test the robustness and reliability of the new generation spectral-line identifier PyEMILI, as initially introduced in Paper I, in line identification and establish a r…

astro-ph.GA2025

LAMOST Medium-resolution Spectroscopic Survey of the Rosette Nebula

Li-Yue Zhang, Chao-Jian Wu, Xuan Fang +4

We report multi-fiber, medium-resolution spectroscopy of the Rosette Nebula with full spatial coverages, and present a table of the nebular parameters based on the spatially-resolv…

astro-ph.GA2025

A Massive Yellow Supergiant in the Far Outer Disk of M31: Evidence for In Situ Massive Star Formation Beyond the Optical Radius

Pinjian Chen, Bingqiu Chen, Haibo Yuan +5

While massive stars are known to shape galactic ecosystems, their formation has long been assumed to require the high-density environments of inner galactic disks. This paradigm is…