activity
20102023
most citedA wide star-black-hole binary system from radial-velocity measurements

200 citations · 879 across the 37 of their papers we have counts for

collaborators
Showing 2022Show all

11 papers · 1 filter

astro-ph.SR2022★ 14 cited

Stellar chromospheric activities revealed from the LAMOST-K2 time-domain survey

Henggeng Han, Song Wang, Yu Bai +3

By using the LAMOST time-domain survey data, we study stellar activities based on the lines for about 2000 stars in four 2 plates. Two indices, and…

astro-ph.HE2022★ 20 cited

Discovery of one neutron star candidate from radial velocity monitoring

Hailong Yuan, Song Wang, Zhongrui Bai +8

We report the discovery of one possible neutron star binary ( 0.8666 day) by using the LAMOST low-resolution spectroscopic data. The visible companion is a late A-ty…

astro-ph.HE2022★ 20 cited

The Nearest Neutron Star Candidate in a Binary Revealed by Optical Time-domain Surveys

Ling-Lin Zheng, Mouyuan Sun, Wei-Min Gu +19

The near-Earth (within pc) supernova explosions in the past several million years can cause the global deposition of radioactive elements (e.g., Fe) on Earth. The…

astro-ph.SR2022★ 12 cited

A White Dwarf-Main Sequence Binary Unveiled by Time-Domain Observations from LAMOST and TESS

Ling-Lin Zheng, Wei-Min Gu, Mouyuan Sun +16

We report a single-lined white dwarf-main sequence binary system, LAMOST J172900.17+652952.8, which is discovered by LAMOST's medium resolution time-domain surveys. The radial velo…

astro-ph.SR2022★ 13 cited

A long-period pre-ELM system discovered from LAMOST medium-resolution survey

Zhi-Xiang Zhang, Ling-Lin Zheng, Wei-Min Gu +16

We present LAMOST~J041920.07+072545.4 (hereafter J0419), a close binary consisting of a bloated extremely low mass pre-white dwarf (pre-ELM WD) and a compact object with an orbital…

astro-ph.SR2022★ 31 cited

A dynamically discovered and characterized non-accreting neutron star -- M dwarf binary candidate

Tuan Yi, Wei-Min Gu, Zhi-Xiang Zhang +26

Optical time-domain surveys can unveil and characterize exciting but less-explored non-accreting and/or non-beaming neutron stars (NS) in binaries. Here we report the discovery of…

astro-ph.SR2022★ 14 cited

Binaries with possible compact components discovered from the LAMOST Time-Domain Survey of four 2 plates

Li Xue, Wang Song, Zhao Xinlin +4

Time-domain (TD) spectroscopic data from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) can provide accurate and high-cadence radial velocities (RVs). In th…

astro-ph.SR2022

Fundamental parameters for dEB SB2 binary system J064726.39+223431.6

Mikhail Kovalev, Song Wang, Xuefei Chen +1

We present a study of eclipsing binary J064726.39+223431.6 using spectra from the LAMOST-MRS and TESS photometry. We use full-spectrum fitting to derive radial velocities and spect…

astro-ph.SR2022★ 21 cited

Probable Dormant Neutron Star in a Short-Period Binary System

Tsevi Mazeh, Simchon Faigler, Dolev Bashi +24

We have identified 2XMM J125556.57+565846.4, at a distance of 600 pc, as a binary system consisting of a normal star and a probable dormant neutron star. Optical spectra exhibit a…

astro-ph.GA2022★ 93 cited

Overview of the LAMOST survey in the first decade

Hongliang Yan, Haining Li, Song Wang +24

The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST), also known as the Guoshoujing Telescope, is a major national scientific facility for astronomical research l…

astro-ph.EP2022★ 6 cited

Detecting and Monitoring Tidal Dissipation of Hot Jupiters in the Era of SiTian

Fan Yang, Wei Wang, Xing Wei +13

Transit Timing Variation (TTV) of hot Jupiters provides direct observational evidence of planet tidal dissipation. Detecting tidal dissipation through TTV needs high precision tran…