The composite image on the left shows an image from NASA's Chandra X-ray
Observatory in purple and an optical image from the European Southern
Observatory's Very Large Telescope (VLT) in red, blue and white. The
Chandra source in the center of the image is the ancient pulsar PSR
J0108-1431 (J0108 for short), located only 770 light years from us. The
elongated object immediately to its upper right is a background galaxy that
is unrelated to the pulsar. Since J0108 is located a long way from the
plane of our galaxy, many distant galaxies are visible in the larger-scale
optical image.
The position of the pulsar seen by Chandra in this image from early 2007 is
slightly different from the radio position observed in early 2001, implying
that the pulsar is moving at a velocity of about 440,000 miles per hour, in
the direction shown by the white arrow. The detection of this motion
allowed an estimate of where J0108 should be located in the VLT image taken
in 2000. The faint blue star just above the galaxy is a possible optical
detection of the pulsar.
The artist's impression on the right shows what J0108 might look like if
viewed up close. Radiation from particles spiraling around magnetic fields is shown along with heated areas around the neutron star's magnetic
poles. Both of these effects are expected to generate X-ray emission. Most
of the surface of the neutron star is expected to be too cool to produce
X-rays, but it should produce optical and ultraviolet radiation. Thus,
multiwavelength observations are important for providing a complete picture
of these exotic objects.
At an age of about 200 million years, this pulsar is the oldest isolated
pulsar ever detected in X-rays. Among isolated pulsars - ones that have not
been spun-up in a binary system - it is over 10 times older than the
previous record holder with an X-ray detection. This pulsar is slowing
down as it ages and converting some of the energy that is being lost into
X-rays. The efficiency of this process for J0108 is found to be higher
than for any other known pulsar.
Fast Facts for PSR J0108-1431: |
Credit |
X-ray: NASA/CXC/Penn State/G.Pavlov et al.; Optical: ESO/VLT/UCL/R.Mignani et al.; Illustration: NASA/CXC/M.Weiss. |
Release Date |
February 26, 2009 |
Scale |
Left panel is 1.3 arcmin across. |
Category |
Neutron Stars/X-ray Binaries |
Coordinates (J2000) |
RA | Dec |
Constellation |
Cetus |
Observation Date |
February 5, 2007
|
Observation Time |
8 hours |
Obs. ID |
7576
|
Instrument |
ACIS
|
References | Pavlov, G., et al., 2009, Astrophysical Journal, 691, 458 |
Color Code |
X-ray (Purple); Optical (Red, Blue, White) |
Distance Estimate |
About 770 light years
|
|