Author
Listed:
- Ji-Feng Liu
(Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences
College of Astronomy and Space Sciences, University of 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
College of Astronomy and Space Sciences, University of Chinese Academy of Sciences)
- You-Jun Lu
(Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences
College of Astronomy and Space Sciences, University of 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
Universidad de la Laguna)
- Pedro Álvarez
(Instituto de Astrofísica de Canarias
Universidad de la Laguna)
- Yi Cao
(Caltech)
- Shri Kulkarni
(Caltech)
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.
Suggested Citation
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 & Shri Kulkarni, 2015.
"Relativistic baryonic jets from an ultraluminous supersoft X-ray source,"
Nature, Nature, vol. 528(7580), pages 108-110, December.
Handle:
RePEc:nat:nature:v:528:y:2015:i:7580:d:10.1038_nature15751
DOI: 10.1038/nature15751
Download full text from publisher
As the access to this document is restricted, you may want to search for a different version of it.
Corrections
All material on this site has been provided by the respective publishers and authors. You can help correct errors and omissions. When requesting a correction, please mention this item's handle: RePEc:nat:nature:v:528:y:2015:i:7580:d:10.1038_nature15751. See general information about how to correct material in RePEc.
If you have authored this item and are not yet registered with RePEc, we encourage you to do it here. This allows to link your profile to this item. It also allows you to accept potential citations to this item that we are uncertain about.
We have no bibliographic references for this item. You can help adding them by using this form .
If you know of missing items citing this one, you can help us creating those links by adding the relevant references in the same way as above, for each refering item. If you are a registered author of this item, you may also want to check the "citations" tab in your RePEc Author Service profile, as there may be some citations waiting for confirmation.
For technical questions regarding this item, or to correct its authors, title, abstract, bibliographic or download information, contact: Sonal Shukla or Springer Nature Abstracting and Indexing (email available below). General contact details of provider: http://www.nature.com .
Please note that corrections may take a couple of weeks to filter through
the various RePEc services.