The Chandra X-ray Observatory. What Are X-Rays?. Chandra: An X-ray Observatory. Chandra in the Space Shuttle. Chandra Launch and Deployment. Launch. Deployment. Chandra Orbit. Chandra: Really in Orbit!. Constellations: Guides to the Sky. Stars Young and Old. Trees Large and Small.By sezja
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Supernova Remnant Group. By: Shakib Ahmed & Al Soedomo The Chandra Astrophysics Institute Lynn English High School. Introduction. How did we get here? Stars go through the “circle of life” Astrophysicists are trying to unravel their behaviors They have made inconceivable progress!.
Spitzer Imaging of Kepler’s Supernova Remnant. W.P. Blair, R. Sankrit, P.Ghavamian (JHU), K.S. Long (STScI), K. Borkowski & S.P. Reynolds (NCSU).
Supernova Remnant Dynamics: Opportunities for Astro-H. Knox S. Long, Aya Bamba And SNR Dynamics WPT. Why observe SNRs with Astro-H – Science. SNRs are particle accelerators and sources of cosmic rays and high energy gamma rays that we do not understand well
50-500 million K Gas. 10 thousand K gas. White Dwarf. Neutron star. Supernova Remnant Cas A, 17-18 light years in diameter. Planetary Nebula Ring Nebula, 1/3 light year diameter. Type II Supernova. Core burns all fuel, from hydrogen all the way to iron: then the star collapses!.
International Conference The Origin and Evolution of Cosmic Magnetism @ Bologna, Italy 2005/8/30. Biermann Mechanism in Primordial Supernova Remnant and Seed Magnetic Fields. ApJ Accepted astro-ph/0501538.
超新星遗迹 supernova remnant ( 简称 SNR) 超新星爆发时遗留的残骸，一般指星云状遗迹。超新星爆发时大质量星的外层或整个炸碎的星向周围空间迅猛地抛出大量物质 , 这些物质在膨胀过程中和星际物质互相作用 , 形成丝状气体云和气壳，遗留在空间 , 成为非热射电源 , 这就是超新星遗迹 ( 简称 SNR) 。现在常用的是 Green D.A. 编写并不断修订的超新星遗迹星表，它包括 231 颗超新星遗迹。表中给出每个超新星遗迹的银道和赤道座标、尺度大小、类型、能流密度和近万篇参考文献。.
High-energy particle acceleration in the shell of a supernova remnant. F.A. Aharonian et al (the HESS Collaboration) Nature 432 , 75 (2004) Nuclear Physics Group Journal Club Jan. 31, 2005 as interpreted by J.W. Martin University of Winnipeg. Cosmic Rays.
OH (1720 MHz) Masers: Tracers of Supernova Remnant / Molecular Cloud Interactions. Crystal L. Brogan (NRAO). VLBA 10 th Anniversary Meeting June 8-12, 2003. The Search for SNR/ Molecular Cloud Interactions. SNRs are one of the most energetically important constituents of the Galactic medium