L
Lijun Gou
Researcher at Chinese Academy of Sciences
Publications - 14
Citations - 411
Lijun Gou is an academic researcher from Chinese Academy of Sciences. The author has contributed to research in topics: Black hole & Gravitational wave. The author has an hindex of 8, co-authored 14 publications receiving 292 citations.
Papers
More filters
Journal ArticleDOI
Cygnus X-1 contains a 21-solar mass black hole-Implications for massive star winds.
James Miller-Jones,Arash Bahramian,Jerome A. Orosz,Ilya Mandel,Ilya Mandel,Ilya Mandel,Lijun Gou,Thomas J. Maccarone,Coenraad J. Neijssel,Coenraad J. Neijssel,Coenraad J. Neijssel,X. H. Zhao,Janusz Ziółkowski,Mark J. Reid,Phil Uttley,Xueying Zheng,Do-Young Byun,Do-Young Byun,Richard Dodson,Victoria Grinberg,Taehyun Jung,Taehyun Jung,Jeong-Sook Kim,Benito Marcote,Sera Markoff,Maria Rioja,Maria Rioja,Maria Rioja,A. Rushton,A. Rushton,David M. Russell,Gregory R. Sivakoff,Alexandra J. Tetarenko,Valeriu Tudose,Joern Wilms +34 more
TL;DR: In this paper, the authors used radio astrometry to refine the distance to the black hole X-ray binary Cygnus X-1, which was found to be 2.22 − 0.17 + 0.18 kiloparsecs.
Journal ArticleDOI
The Mass of the Black Hole in the X-ray Binary Nova Muscae 1991
Zihan Chen,Lijun Gou,Jeffrey E. McClintock,James F. Steiner,Jianfeng Wu,Weiwei Xu,Jerome A. Orosz,Yanmei Xiang,Yanmei Xiang +8 more
TL;DR: In this paper, it was shown that the optical counterpart of the black-hole soft X-ray transients in quiescence occurs at a nearly linear rat e. This discovery, and precise determination of the disk component of emission obtained using our simultaneousphotometric and spectroscopic data, have allowed us to identify and accurately model archival ellipsoidal light curves of the highest quality.
Journal ArticleDOI
Constraining Cosmological Parameters in the FLRW Metric with Lensed GW+EM Signals
TL;DR: In this paper, a model-independent method to constrain cosmological parameters using the distance sum rule of the Friedmann-Lemaitre-Robertson-Walker metric was proposed.
Proceedings ArticleDOI
Measuring the Spins of Stellar Black Holes: A Progress Report
TL;DR: In this paper, the authors used the Novikov-thorne thin disk model to fit the thermal continuum X-ray spectra of black hole X−ray binaries, and extracted the dimensionless spin parameter a* √ m/m of the black hole as a parameter of the fit.