activity
20092023
most citedDiscovery of the transient magnetar 3XMM J185246.6+003317 near supernova remnant Kesteven 79 with XMM-Newton

53 citations · 134 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.EP2023★ 1 cited

Dynamical Stability of Polar Circumbinary Orbits and Planet-Formation in Planetary Disc of 99 Herculis

Ying Wang, Wei Sun, Ji-lin Zhou +2

A possible polar-ring debris disc, the dynamics of which can be described by the outer hierarchical restricted three-body problem, has been detected in 99 Herculis. An empirical fo…

astro-ph.HE2022★ 9 cited

CHANG-ES XXIX: The Sub-kpc Nuclear Bubble of NGC 4438

Jiang-Tao Li, Q. Daniel Wang, Theresa Wiegert +8

AGN bubbles could play an important role in accelerating high-energy CRs and galactic feedback. Only in nearby galaxies could we have high enough angular resolution in multi-wavele…

astro-ph.GA2022★ 4 cited

X-ray Spectroscopic Evidence of Charge Exchange Emission in the Disk of M51

Shuinai Zhang, Q. Daniel Wang, Wei Sun +3

In the disks of spiral galaxies, diffuse soft X-ray emission is known to be strongly correlated with star-forming regions. However, this emission is not simply from a thermal-equil…

astro-ph.GA2022★ 9 cited

CHANG-ES. XXIV. First Detection of A Radio Nuclear Ring and Potential LLAGN in NGC 5792

Yang Yang, Judith Irwin, Jiangtao Li +8

We report the discoveries of a nuclear ring of diameter 10$\arcsec$ (1.5 kpc) and a potential low luminosity active galactic nucleus (LLAGN) in the radio continuum emission m…

astro-ph.IM2020★ 1 cited

Mapping Diffuse Emission in Lyman UV band

Li Ji, Zheng Lou, Jinlong Zhang +38

The CAFE (Census of warm-hot intergalactic medium, Accretion, and Feedback Explorer) and LyRIC (Lyman UV Radiation from Interstellar medium and Circum-galactic medium) have been pr…

astro-ph.GA2019★ 13 cited

XMM-Newton RGS spectroscopy of the M31 bulge. I: Evidences for a past AGN half a million years ago

Shuinai Zhang, Q. Daniel Wang, Adam R. Foster +3

Existing analysis based on XMM-Newton/RGS spectra already shows that the G-ratio of the OVII He triplet in the inner bulge of M31 is too high to be consistent with a pure optica…