activity
20172020
most citedA Catalog of Short Period Spectroscopic and Eclipsing Binaries Identified from the LAMOST & PTF Surveys

17 citations · 46 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.GA20202 cited

Galaxy Optical Variability of Virgo Cluster: New Tracer for Environmental Influences on Galaxies

Fan Yang, Richard J. Long, Su-Su Shan +6

We investigate the relationship between the optical variability of galaxies and their distances from the centre of the Virgo Cluster using Palomar Transient Factory data. We define…

astro-ph.SR202017 cited

A Catalog of Short Period Spectroscopic and Eclipsing Binaries Identified from the LAMOST & PTF Surveys

Fan Yang, Richard J. Long, Su-Su Shan +7

Binaries play key roles in determining stellar parameters and exploring stellar evolution models. We build a catalog of 88 eclipsing binaries with spectroscopic information, taking…

astro-ph.GA2019

The kinematic distances of SNR G16.7+0.1 and G15.9+0.2 by analyzing HI absorption spectra

W. W. Tian, H. Zhu, M. F. Zhang +3

We build HI absorption spectra towards Supernova Remnant (SNRs) G16.7+0.1 and G15.9+0.2 using the THOR survey data. With the absorption spectra, we give a new distance range of 7 t…

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.IM2018

Distances of Galactic Supernova Remnants Using Red Clump Stars

S. S. Shan, H. Zhu, W. W. Tian +4

We carry out a project to independently measure the distances of supernova remnants (SNRs) in the first quadrant of the Galaxy. In this project, red clump (RC) stars are used as st…

astro-ph.GA201711 cited

Disentangling the radio emission of the supernova remnant W51C

M. F. Zhang, W. W. Tian, D. A. Leahy +3

We simulate the evolution of supernova remnant (SNR) W51C. The simulation shows the existence of a new northeast edge. We present magnetic field structure of the W51 complex (SNR W…