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XTE J1550-564: A superluminal ejection during the September 1998 outburst
Astrophysics · Submitted 2 Nov 2000
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim The components observed have an apparent separation velocity of >2c.
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The abstract, sentence by sentence
In 1998 September, the X-ray transient XTE J1550-564 underwent a major outburst in soft and hard X-rays, followed by a radio flare. Australian Long Baseline Array images obtained shortly after the peak in the radio flare showed evolving structure. The components observed have an apparent separation velocity of >2c.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | In 1998 September, the X-ray transient XTE J1550-564 underwent a major outburst in soft and hard X-rays, followed by a radio flare. | background 0.78 | 0.40 | 0.05 | asserted 1.00 |
| s1 | Australian Long Baseline Array images obtained shortly after the peak in the radio flare showed evolving structure. | method 0.85 | 0.79 | 0.04 | asserted 1.00 |
| s2 | The components observed have an apparent separation velocity of >2c. | result 1.00 | 0.84 | 0.76 | asserted 1.00 |
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The paper
Original abstract
In 1998 September, the X-ray transient XTE J1550-564 underwent a major outburst in soft and hard X-rays, followed by a radio flare. Australian Long Baseline Array images obtained shortly after the peak in the radio flare showed evolving structure. The components observed have an apparent separation velocity of >2c.
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1 arXiv paper cite this in 1 sentence
Papers whose main result relates to this one's
States the same result 1 paper
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The apparent separation velocity of the two outermost components is v>2c.
Radio Emission from the X-ray transient XTE J1550-564 · 1.00
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