A new, faint population of X-ray transients

F. E. Bauer(Space Science Institute), Guang Yang(University of Groningen), Д. А. Канн(Thüringer Landessternwarte Tautenburg), P. Tozzi(Arcetri Astrophysical Observatory), Junxian Wang(University of Science and Technology of China), W. N. Brandt, C. Vignali(Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna), F. Förster(Universidad de Santiago de Chile), K. Nomoto(Kavli Institute for the Physics and Mathematics of the Universe), Yongquan Xue(University of Science and Technology of China), Ohad Shemmer, Alexey Tolstov(Kavli Institute for the Physics and Mathematics of the Universe), A. Comastri(Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna), Keiichi Maeda(Kyoto University), Kevin Schawinski(ETH Zurich), S. Schulze(Northwestern University), Bin Luo(Nanjing University), P. Ranalli(Lund University), R. Gilli(Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna), M. Paolillo(Agenzia Spaziale Italiana), Masaomi Tanaka(National Astronomical Observatory of Japan), Ezequiel Treister(Pontificia Universidad Católica de Chile), Nozomu Tominaga(Institució Catalana de Recerca i Estudis Avançats), Donald P. Schneider(Russian State University for the Humanities)
Monthly Notices of the Royal Astronomical Society
February 17, 2017
Cited by 91


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