News by Date
News by Category
Solar System
White Dwarfs
Neutron Stars
Black Holes
Milky Way Galaxy
Normal Galaxies
Galaxy Clusters
Cosmology/Deep Field
Press Resources
Status Reports
Press Advisories
Image Releases
Release Guidelines
Image Use Policy
Web Shortcuts
Chandra Blog
RSS Feed
Email Newsletter
News & Noteworthy
Image Use Policy
Questions & Answers
Glossary of Terms
Download Guide
Get Adobe Reader
Related Links

Chandra @ NASA
Visit the Chandra pages at the NASA portal (opens in new window)
Image Use
Image Use Policy & Request Form
Guidelines for utilizing images, applets, movies, and animations featured in this Web Site.
Pulsar Punches Hole In Stellar Disk

For Release: July 22, 2015


X-ray: NASA/CXC/PSU/G.Pavlov et al; Illustration: NASA/CXC/M.Weiss

A fast-moving pulsar appears to have punched a hole in a disk of gas around its companion star and launched a fragment of the disk outward at a speed of about 40 million miles per hour. NASA’s Chandra X-ray Observatory is tracking this cosmic clump, which appears to be picking up speed as it moves out.

The double star system PSR B1259-63/LS 2883 – or B1259 for short – contains a star about 30 times as massive as the Sun and a pulsar, an ultra-dense neutron star left behind when an even more massive star underwent a supernova explosion.

The pulsar emits regular pulses as it spins 20 times a second, and moves in a highly elliptical orbit around its companion star. The combination of rapid rotation and intense magnetic field of the pulsar has generated a strong wind of high-energy particles moving away from the pulsar at near the speed of light.

The massive companion star, meanwhile, is rotating close to break-up speed and is spinning off a disk of material. As the pulsar makes its closest approach to the star every 41 months, it passes through this disk

“These two objects are in an unusual cosmic arrangement and have given us a chance to witness something special,” said George Pavlov of Penn State University in State College, Pennsylvania, lead author of a paper describing these results. “As the pulsar moved through the disk, it appears that it punched a clump of material out and flung it away into space.” 

Even though the clump is rather large, spanning a hundred times the size of our Solar System, it is also quite thin. The material in it has the mass equivalent to all the water in the Earth’s oceans.

“After this clump of stellar material was knocked out, the pulsar’s wind appears to have accelerated it, almost as if it had a rocket attached,” said co-author Oleg Kargaltsev of George Washington University (GWU) in Washington, DC.

Astronomers observed B1259, which is located about 7,500 light years from Earth, three times with Chandra between December 2011 and February 2014. These observations show the clump moving away from B1259 at an average speed of about 7% of the speed of light. The data also indicate that the clump has been accelerated to 15% of the speed of light between the second and third observations.

“This just shows how powerful the wind blasting off a pulsar can be,” said co-author Jeremy Hare, also of GWU. “The pulsar’s wind is so strong that it could ultimately eviscerate the entire disk around its companion star over time.”

The X-ray emission observed by Chandra is likely produced by a shock wave created as the pulsar’s wind rams into the clump of material. The ram pressure generated by this interaction could also accelerate the clump.

Chandra will continue monitoring B1259 and its moving clump with observations scheduled for later this year and in 2016.

These results appeared in the June 20, 2015 issue of The Astrophysical Journal and are available online. NASA's Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, controls Chandra's science and flight operations.

Media contacts:
Megan Watzke
Chandra X-ray Center, Cambridge, Mass.

Visitor Comments (4)

I feel it's so difficult to understand, if this can change to Chinese will be better. My English is poor.

Posted by Anne on Tuesday, 09.22.15 @ 10:16am

If the neutron star has a period of 41 months why has it not disturbed the decretion disc on previous orbits, giving rise to earlier ejection?

Posted by Dr Clive L. Fetter on Monday, 07.27.15 @ 04:59am

This didn't tell me much information that I was actually looking for. I was hoping that this article would have went into more detail about this neutron star and this other host star colliding and ejecting some mass amount of stellar debris into space. I love reading ALL articles of the Chandra observatory and the Hubble space telescope, I am a huge fan of cosmology, astronomy, physics, etc I just wished they had released more information on this article than what NASA actually released. I know they have more info than what they actually released.

Posted by Jason Jenkins on Thursday, 07.23.15 @ 01:01am

Does this impose any threat to us on earth?

Posted by Rick on Wednesday, 07.22.15 @ 22:07pm