Images by Date
Images by Category
Solar System
Stars
White Dwarfs
Supernovas
Neutron Stars
Black Holes
Milky Way Galaxy
Normal Galaxies
Quasars
Galaxy Clusters
Cosmology/Deep Field
Miscellaneous
Images by Interest
Space Scoop for Kids
4K JPG
Multiwavelength
Sky Map
Constellations
3D Wall
Photo Blog
Top Rated Images
Image Handouts
Desktops
High Res Prints
Fits Files
Image Tutorials
Photo Album Tutorial
False Color
Cosmic Distance
Look-Back Time
Scale & Distance
Angular Measurement
Images & Processing
AVM/Metadata
Getting Hard Copies
Image Use Policy
Web Shortcuts
Chandra Blog
RSS Feed
Chronicle
Email Newsletter
News & Noteworthy
Image Use Policy
Questions & Answers
Glossary of Terms
Download Guide
Get Adobe Reader
PSR B1259-63: Pulsar Punches Hole In Stellar Disk
PSR B1259-63
PSR B1259-63
PSR B1259-63
PSR B1259-63

  • A clump of material has been jettisoned from a double star system at incredibly high speeds.

  • X-rays from Chandra reveal that a pulsar in orbit around a massive star punched through a circumstellar disk of material.

  • Three Chandra observations of the system were taken between December 2011 and February 2014.

  • The data suggest the clump may even be accelerating due to the pulsar's powerful winds.


This trio of images contains evidence from NASA's Chandra X-ray Observatory that a clump of stellar material has been jettisoned away from a double star system at incredibly high speeds. This system, known as PSR B1259-63/LS 2883 – or B1259 for short – is comprised of two objects in orbit around one another. The first is a star about 30 times as massive as the Sun that has a disk of material swirling around it. The other is a pulsar, an ultra-dense neutron star left behind when an even more massive star underwent a supernova explosion.

Researchers think that the pulsar knocked out the chunk of debris, which spans over a hundred times the size of the Solar System, when it collided with the disk around the massive star while traveling in its elliptical orbit lasting 41 months. (An artist's illustration shows the pulsar just after having collided with the disk.) Astronomers came to this conclusion after analyzing three separate Chandra observations taken between December 2011 and February 2014, as labeled in the three images. The bright source in the center of these images is the binary system, while the smaller point-like source to the lower right seen in the second two observations is the clump that has been dislodged.

The Chandra observations also suggest that the clump is not only moving quickly but may, in fact, be picking up speed. The average of the three observations shows the clump is moving about 7% the speed of light, but the data suggest it may have accelerated to 15% the speed of light between the second and third observations. This acceleration could be due to intense winds flowing off of the pulsar's surface at nearly the speed of light, which are caused by its rapid rotation and strong magnetic fields.

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. The authors of this paper are George Pavlov (Penn State University), Jeremy Hare (George Washington University), Oleg Kargaltsev (George Washington University), Blagory Rangelov (George Washington University), and Martin Durant (University of Florida).

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.

Fast Facts for PSR B1259-63:
Credit  X-ray: NASA/CXC/PSU/G.Pavlov et al; Illustration: NASA/CXC/M.Weiss
Release Date  July 22, 2015
Scale  Image is about 40 arcsec across (1.3 light years)
Category  Neutron Stars/X-ray Binaries
Coordinates (J2000)  RA 13 02 47.60 | Dec -63 50 08.70
Constellation  Centaurus
Observation Date  4 pointings: 12/17/2011, 05/19/2013, 02/08 and 02/09/2014
Observation Time  1 day 46 min (42 hours 46 min)
Obs. ID  14205, 14206, 16563, 16583
Instrument  ACIS
References Pavlov, G et al, 2015, ApJ, 806, 192; arXiv:1505.07155
Color Code  X-ray: Blue
X-ray
Distance Estimate  About 7,500 light years
distance arrow
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


Leave Your Comment


 
 

Rules

Rate This Image

Rating: 3.9/5
(293 votes cast)
Download & Share

More Information
Press Room: PSR B1259-63
Blog: PSR B1259-63
More Images
X-ray Image of PSR B1259-63
Jpg, Tif
X-ray

More Images
Animation & Video
Tour of PSR B1259
animation

More Animations
Related Images
G327.1-1.1
G327.1-1.1
(19 Nov 14)

The Eagle Nebula M16
IGR J11014-6103
(18 Feb 14)

Related Information
Related Podcast
Top Rated Images
GOODS-S 29323

GRB 140903A

TW Hya Association




FaceBookTwitterYouTubeFlickr