activity
20172021
most citedThe gas-to-extinction ratio and the gas distribution in the Galaxy

114 citations · 136 across the 3 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2021

A Supernova-driven, Magnetically-collimated Outflow as the Origin of the Galactic Center Radio Bubbles

Mengfei Zhang, Zhiyuan Li, Mark R. Morris

A pair of non-thermal radio bubbles recently discovered in the inner few hundred parsecs of the Galactic center bears a close spatial association with elongated, thermal X-ray feat…

astro-ph.GA2020

Extended radio AGN at z ~ 1 in the ORELSE survey: The confining effect of dense environments

Lu Shen, Guilin Liu, Mengfei Zhang +16

Recent hydrodynamic simulations and observations of radio jets have shown that the surrounding environment has a large effect on their resulting morphology. To investigate this we…

astro-ph.HE2020

Galactic Center IRS13E: Colliding Stellar Winds or an Intermediate Mass Black Hole?

Zhenlin Zhu, Zhiyuan Li, Anna Ciurlo +4

A small cluster of massive stars residing in the Galactic center, collectively known as IRS13E, is of special interest due to its close proximity to Sgr A* and the possibility that…

astro-ph.GA201916 cited

The Distance Measurements of Supernova Remnants in The Fourth Galactic Quadrant

Su-Su Shan, Hui Zhu, Wen-Wu Tian +3

We take advantage of the red clump stars to build the relation of the optical extinction (AV) and distance in each direction of supernova remnants (SNRs) with known extinction in t…

astro-ph.GA2018

How does the stellar wind influence the radio morphology of a supernova remnant?

M. F. Zhang, W. W. Tian, D. Wu

We simulate the evolutions of the stellar wind and the supernova remnant (SNR) originating from a runaway massive star in an uniform Galactic environment based on the three-dimensi…

astro-ph.GA2017114 cited

The gas-to-extinction ratio and the gas distribution in the Galaxy

Hui Zhu, Wenwu Tian, Aigen Li +1

We investigate the relation between the optical extinction () and the hydrogen column density () determined from X-ray observations of a large sample of Galactic sightlin…