The Isolated Neutron Star RX J185635-3754
[November 2000]
Hubble Space Telescope observations of the isolated neutron star
RX J185635-3754 have now revealed its distance and its motion across
the sky. This object, the brightest isolated (non-pulsing) neutron star known,
was discovered in 1992 from its intense X-ray emission (Walter, Wolk, &
Neuhaeuser, Nature 379, 233, 1996). The optical counterpart, a faint blue
star, was discovered in Hubble Space Telescope images obtained in October
1996 (Walter & Matthews, Nature 389, 358, 1997; image and press release
available at http://oposite.stsci.edu/pubinfo/pr/97/32.html). Two
additional images obtained in 1999 wave show that the neutron star is located
at a distance of 61 parsecs (200 light years), and that it is moving through
space with a velocity of 108 km/s. This is the closest known neutron star to
the Earth. The direction of motion suggests that it was ejected from the
Upper Scorpius association about 900,000 years ago, about the same time when a
supernova is known to have gone off there (neutron stars are created in
supernova explosions). This work will appear in the Astrophysical Journal
(March 2001), and the press release is available at
http://oposite.stsci.edu/pubinfo/PR/2000/35/index.html.
Neutron stars are the densest form of matter known in the universe, and
provide a testbed for theories of matter at high densities.
Stony Brook astronomers will continue to observe RX J185635-3754 with
the Hubble Space Telescope and the Chandra X-ray Observatory, in order to
further study the composition and equation of state of this neutron star.