HEAPOW: Silent Superball (2011 Mar 07)
Cassiopeia A: Chandra Finds Superfluid in Neutron Star's CoreLight from a massive star, which blew up about 11,000 years ago, first reached earth about 3 centuries ago. Though the explosion was extremely powerful, and must have been incredibly luminous, the event was not recorded until 1947 when radio emission from the glowing gases ejected in the explosion was first detected. Since then, this remnant has been known as the Cas A supernova remnant, and is an object of intense scrutiny by astronomers. The ejecta produces not only strong radio emission but strong X-ray emission as well. Models of such stellar explosions predict that a strange chunk of matter, a neutron star or black hole, should be left behind in the middle of the remnant. But this object went undetected for about 50 years, until 1999 when the Chandra X-ray Telescope, with its incredible mirrors, was able to pinpoint the X-ray glow from the object cleanly resolved from the complex glowing bright emission around it. The Chandra X-ray image of Cas A is shown above; the strange chunk left behind, a ball which could fit comfortably inside the Washington DC beltway, is marked by a box and shown in the artist conception on the lower right. Thanks to Chandra, astronomers now know that this super-ball is a silent, non-pulsating neutron star, an object with a crust of solid iron, surrounded by an inches-thick carbon atmosphere denser than diamond. But what lies beneath is even more amazing. The rapid cooling of the neutron star as measured by Chandra over the last decade means that the neutron star must have a core of superfluid neutrons, a state of matter never before observed in the Universe.
http://asterisk.apod.com/viewtopic.php?f=31&t=22852
APOD: Cooling Neutron Star (2011 Mar 05)
http://asterisk.apod.com/viewtopic.php?f=9&t=23082
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Author: Dr. Michael F. Corcoran
A service of the Astrophysics Science Division (ASD) at NASA/GSFC and the
High Energy Astrophysics Division of the Smithsonian Astrophysical Observatory (SAO)
A service of the Astrophysics Science Division (ASD) at NASA/GSFC and the
High Energy Astrophysics Division of the Smithsonian Astrophysical Observatory (SAO)