105 citations · 151 across the 7 of their papers we have counts for
7 papers
Self-consistent Stellar Radial Velocities from LAMOST Medium-Resolution Survey (MRS) DR7
Bo Zhang, Jiao Li, Fan Yang +12
Radial velocity (RV) is among the most fundamental physical quantities obtainable from stellar spectra and is rather important in the analysis of time-domain phenomena. The LAMOST…
Comprehensive Photometric Investigation of an Active Early K-type Contact System -- IL Cnc
N. -P. Liu, T. Sarotsakuchai, S. Rattanasoon +1
Comprehensive photometric investigation was carried out to the early K-type contact binary - IL Cnc. A few light curves from both ground-based telescopes and the Kepler space teles…
New Photometric Investigation of the Low-Mass-Ratio Contact Binary Star V1853 Orionis
Jia-Jia He, Sheng-Bang Qian, B. Soonthornthum +3
Four-color charge-coupled device (CCD) light curves in , , and bands of the total-eclipsing binary system, V1853 Ori, are presented. By comparing our light curves w…
Formation of the Abundance Boundaries of the Heavier Neutron-capture Elements in Metal-poor Stars
Guochao Yang, Hongjie Li, Nian Liu +5
The abundance scatter of heavier r-process elements (Z > 56) relative to Fe ([r/Fe]) in metal-poor stars preserves excellent information of the star formation history and provides…
Footprints of the weak s-process in the carbon-enhanced metal-poor star ET0097
Guochao Yang, Hongjie Li, Nian Liu +3
Historically, the weak s-process contribution to metal-poor stars is thought to be extremely small, due to the effect of the secondary-like nature of the neutron source 22Ne(a;n)25…
Photometric Investigation of the K-type Extreme-Shallow Contact Binary V1799 Orion
Nian-Ping Liu, Sheng-Bang Qian, Wen-Ping Liao +3
New multi-color light curves of the very short period K-type eclipsing binary V1799 Ori were obtained and analyzed with the W-D code. The photometric solutions reveal that the syst…
AE Ursae Majoris -- a Scuti Star in the Hertzsprung Gap
Jia-Shu Niu, Jian-Ning Fu, Yan Li +7
We analyze the photometric data and spectroscopic data that collect on the Scuti star AE UMa. The fundamental and the first overtone frequencies are confirmed as $f_{0} = 11.62…