Relativistic baryonic jets from an ultraluminous supersoft X-ray source
Ji-Feng Liu (),
Yu Bai,
Song Wang,
Stephen Justham,
You-Jun Lu,
Wei-Min Gu,
Qing-Zhong Liu,
Rosanne Di Stefano,
Jin-Cheng Guo,
Antonio Cabrera-Lavers,
Pedro Álvarez,
Yi Cao and
Shri Kulkarni
Additional contact information
Ji-Feng Liu: Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences
Yu Bai: Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences
Song Wang: Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences
Stephen Justham: Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences
You-Jun Lu: Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences
Wei-Min Gu: Xiamen University
Qing-Zhong Liu: Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences
Rosanne Di Stefano: Harvard-Smithsonian Center for Astrophysics
Jin-Cheng Guo: Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences
Antonio Cabrera-Lavers: Instituto de Astrofísica de Canarias
Pedro Álvarez: Instituto de Astrofísica de Canarias
Yi Cao: Caltech
Shri Kulkarni: Caltech
Nature, 2015, vol. 528, issue 7580, 108-110
Abstract:
Persistent low-velocity baryonic jets have been detected from a supersoft X-ray source; the low velocity suggests that these jets have not been launched from a white dwarf, and the persistence speaks against the origin being a canonical black hole or neutron star, indicating that a different type of source must be implicated.
Date: 2015
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DOI: 10.1038/nature15751
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