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20062023
most citedA wide star-black-hole binary system from radial-velocity measurements

200 citations · 1.1k across the 32 of their papers we have counts for

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10 papers · 1 filter

astro-ph.SR2021★ 9 cited

The Data Processing of the LAMOST Medium-Resolution Spectral Survey of Galactic Nebulae (LAMOST MRS-N Pipeline)

Chao-Jian Wu, Hong Wu, Wei Zhang +8

The Large sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) medium-resolution spectral survey of Galactic Nebulae (MRS-N) has conducted for three years since Sep. 2018 a…

astro-ph.SR2020★ 9 cited

A New Transition Wolf-Rayet WN/C Star in the Milky Way

Wei Zhang, Helge Todt, Hong Wu +7

We report the discovery of a new transition type Wolf-Rayet (WR) WN/C star in the Galaxy. According to its coordinates (R.A., Dec)J2000 = 18h51m39.7s, -05d34m51.1s, and the distanc…

astro-ph.SR2020★ 14 cited

On the radial velocity calibrations in the LAMOST Medium-Resolution Spectroscopic Survey of Nebulae

Juan-Juan Ren, Hong Wu, Chao-Jian Wu +12

Accurate radial velocity determinations of optical emission lines (i.e. [NII]6548,6584, H, and [SII]6717,6731) are very important for investigating the kinematics and dy…

astro-ph.SR2020★ 45 cited

LAMOST Medium-Resolution Spectroscopic Survey (LAMOST-MRS): Scientific goals and survey plan

Chao Liu, Jianning Fu, Jianrong Shi +38

Since September 2018, LAMOST starts a new 5-year medium-resolution spectroscopic survey (MRS) using bright/gray nights. We present the scientific goals of LAMOST-MRS and propose a…

astro-ph.SR2019★ 200 cited

A wide star-black-hole binary system from radial-velocity measurements

Jifeng Liu, Haotong Zhang, Andrew W. Howard +52

All stellar mass black holes have hitherto been identified by X-rays emitted by gas that is accreting onto the black hole from a companion star. These systems are all binaries with…

astro-ph.SR2019★ 4 cited

Irregular changes in Hα emission line of V423 Aur observed by LAMOST Medium-Resolution Spectrographs

Chao-Jian Wu, Hong Wu, Chih-Hao Hsia +8

We obtained 7 spectra of the Be star V423 Aur on Dec. 5th, 2017 using the LAMOST Medium-Resolution Spectrograph with exposures from 600 to 1200 seconds. These spectra show the irre…