The X-ray glow keeps growing after the recent neutron star collision | Science News

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The X-ray glow keeps growing after the recent neutron star collision

Puzzled scientists expected the brightness to fade quickly

By
9:00am, January 24, 2018
illustration of neutron star collision

ENDURING LIGHT  X-rays generated in the collision of two neutron stars (illustrated) have unexpectedly gotten brighter over time. Scientists are still trying to understand how jets spewing out from the collision could have produced the long-lasting glow.

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More than 100 days after two neutron stars slammed together, merging into one, new telescope images have revealed that the collision’s lingering X-ray light show has gotten brighter. And scientists don’t fully understand why.

NASA’s orbiting X-ray telescope, Chandra, previously picked up the X-rays 15 days after gravitational waves from the cataclysm reached Earth on August 17, 2017 (SN: 11/11/17, p. 6). The merged remnant then spent several months too close to the sun for its X-rays to be seen.

When the remnant reemerged from the sun’s veil on December 4, it was about four times brighter than when it was last spotted, Daryl Haggard of McGill University in Montreal and her colleagues report January 18 in Astrophysical Journal Letters.

The glow may be tapering off. The XMM-Newton space telescope found on December 29 that the X-ray signal may be starting to weaken, according to a paper published January 18 at arXiv.org.

“The plot is about to thicken,” says Haggard. Chandra has collected new data to look for a drop in brightness.

Scientists are debating how to explain the enduring X-rays. Neutron star collisions are expected to emit bright jets of material, creating X-rays that fade quickly. The long-lasting X-rays might be explained by a “cocoon” of debris (SN Online: 12/20/17), among other possibilities.

Citations

J.J. Ruan et al. Brightening X-Ray emission from GW170817/GRB 170817A: Further evidence for an outflow. Astrophysical Journal Letters. Vol. 853, January 18, 2018, p. L4. doi: 10.3847/2041-8213/aaa4f3.

P. D'Avanzo et al. Evidence for a decreasing X–ray afterglow emission of GW 170817A / GRB 170817A in XMM-Newton observations. arXiv:1801.06164. Posted January 18, 2018.

Further Reading

L. Grossman. Smothered jet may explain weird light from neutron star crash. Science News Online December 20, 2017.

E. Conover. Neutron star collision showers the universe with a wealth of discoveries. Science News. Vol. 192, November 11, 2017, p. 6.

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