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A Possible X-Ray Counterpart to SGR 1900+14

  • Published:1996-05-20 Issue:1 Volume:463 Page:L13-L16
  • ISSN:0004-637X
  • Container-title:The Astrophysical Journal
  • language:
  • Short-container-title:

Author:

Hurley K.,Li P.,Vrba F.,Luginbuhl C.,Hartmann D.,Kouveliotou C.,Meegan C.,Fishman G.,Kulkarni S.,Frail D.,Bowyer S.,Lampton M.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 24 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. CHANDRAASTROMETRY SETS A TIGHT UPPER LIMIT TO THE PROPER MOTION OF SGR 1900+14;The Astrophysical Journal;2009-02-10

2. CONSTRAINING THE PROPER MOTIONS OF TWO MAGNETARS;The Astronomical Journal;2008-12-15

3. QED can explain the non-thermal emission from SGRs and AXPs: variability;Astrophysics and Space Science;2007-03-21

4. QED can explain the non-thermal emission from SGRs and AXPs: variability;Isolated Neutron Stars: From the Surface to the Interior;2007

5. The broad-band spectrum of the persistent emission from SGR 1806-20;Astronomy & Astrophysics;2005-03-22
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