This is Dave Green's Galactic supernova remnant catalogue, or catalog of SNRs, updated 2001 December, containing 231 supernova remnants ...

Cosmic Search Vol. 1, No. 1 Little Green Men, White Dwarfs or Pulsars By S. Jocelyn Bell Burnell We did all the work ourselves and cheerfully sledgehammered all one summer. Burnell and the antenna. In all the history of radio astronomy the pulsing signals discovered at Cambridge, England, in 1967 were the most suggestive of an extraterrestrial intelligent origin that have ever been detected. In ...

Chandra Associates Pulsar and Historic Supernova January 10, 2001 CXC PR: 01-02 Dolores Beasley NASA HQ Phone: 202-358-1753 Steve Roy Marshall Space Flight Center, Huntsville, AL Phone: 256-544-6535 Megan Watzke Chandra X-ray Observatory Center, CFA, Cambridge, MA Phone: 617-496-7998 cxcpress@cfa.harvard.edu Press Image and Caption SAN DIEGO -- Scientists using NASA s Chandra X-ray Observatory ...

Introduction to Pulsar Astronomy A Tutorial on Radio Pulsars This tutorial was produced as part of the lecture course given to MSc students at Jodrell bank in 1996. Pulsar Astronomy This short lecture course was given to 4-year students at the University of Manchester within the Frontier of Astrophysics series in February 2001. The Sounds of Pulsars Listen to the sounds made by the brightest ...

NEUTRON STAR (THEORY) GROUP at UNAM Faculties: Dany Pierre PAGE page@astroscu.unam.mx William LEE ALARDIN wlee@astroscu.unam.mx Students: Armando ROJAS NINO rojas@astroscu.unam.mx Carlos PEREZ TORRES capeto@astroscu.unam.mx Enrique MORENO emoreno@astroscu.unam.mx The Neutron Star Builder Tool-Kit (not yet available) The Neutron Star Cooler Tool-Kit The Neutron Star Picture Gallery Observational ...

This site is intended for students age 14 and up, and for anyone interested in learning about our universe.

Neutron Stars Neutron Stars are the end point of a massive star's life. When a really massive star runs out of nuclear fuel in its core the core begins to collapse under gravity. When the core collapses the entire star collapses. The surface of the star falls down unti l it hits the now incredibly dense core. It then bounces off the core and blows apart in a supernova. All that remains is the ...