PPT-A Chandra view to Exploding Stars

SN2014J R Margutti Harvard nothing Margutti 13 14 Kamble 13 Soderberg 06 10 Energy partitioning SNe are an OPTICAL phenomenon 10 51 erg OPTICAL 10 47 erg XraysRadio. ST5. Training. Exploding assemblies. Course overview. The Explode-Render-Animate application within the Solid Edge assembly environment is a tool for creating different types of presentations of Solid Edge assemblies. Exploding an assembly allows you to control the movement, sequence and grouping of parts and subassemblies. Rendering a view allows you to define textures, lighting, shadows, backgrounds and other properties to create presentation style images. Motors apply movement to under constrained parts in an assembly which can be animated. Using Animation, you can combine previously created exploding sequences and custom camera movement to create animation. Each frame of the animation can be rendered to create presentation quality animations.. Manjil P. Saikia. Department of Mathematical Sciences,. School of Science and Technology,. Tezpur University, India. The Man. and. The Machine. Manjil P. Saikia. 2. Manjil P. Saikia. 3. Chandra can observe X-rays from particles up to the last second before they fall into a black hole!!!. Ian Evans. On behalf of the Chandra Source Catalog Project Team. Chandra Users’ Committee Meeting. October 23, 2014. Summary. Summary of Progress Since . Last CUC . Meeting and Future Plan. Completed algorithm development and implementation through source detection and evaluation (through “. MSc. .. HUKUM MARITIM. FAKULTAS HUKUM UNIVERSITAS INDONESIA. LEGAL REGIME / LIABILITY. (REGIME HUKUM / TANGGUNG JAWAB ). Kitab Undang-Undang Hukum Dagang Indonesia (KUHD). The Hague of Rules. The Hamburg Rules. Ewan O’Sullivan (SAO). thanks to: J. . Vrtilek. ,. L. David, S. . Giacintucci. , S. . Raychaudhury. , A. . Zezas. ,. . and others. How . i. s the hot Intra-Group Medium formed?. Boston, 20 Nov 2014. K-band. 0.5-2 keV. X-ray Emission Line Spectroscopy of Diffuse Hot Plasma. XMM-Newton RGS. Liu, Wang, Li, & Peterson 2010. Li & Wan 2007. T ~ 3 . x. 10. 6. K . Lx. ~2x10. 38. erg/. s. Chandra ACIS-I. Una Hwang (NASA/GSFC, JHU). &. J Martin Laming (NRL). Boston AAS 24 May 2011. Cas A First-light Chandra image (Hughes+ 2000). Red: Fe. , . Green: Si . Cassiopeia A. . Core-collapse SNR with the most prominent Fe ejecta emission. Progenitors and Explosions of Type . Ia. Supernovae. Keiichi Maeda (Kyoto U.). Progenitors – which or even something else?. Double Degenerate (DD. ). WD + WD. Single Degenerate (SD. ). WD + MS/RG. The “. Cosmic Distance Ladder. ”. Visual. “. Parallax. ”. “. Binocular. Vision”…. Let’s us “see” 3D images . (depth). …but, how to do this to get . Astronomical Distances. ?. “. Stars 1. Patterns of stars – constellations a. Ancient cultures used mythology or everyday items to name constellations 2. Modern astronomy studies 88 constellations 3. Some constellations are not ! and I felt myself exploding. Excerpt from an Interview with Marvin Gaye Photo Credit: Billboard, April 27, 1974, Public DomainÒI remember I was listening to a tune of mine playing on the radio Tip 16 copper skin tonestars 2105-8507SMnBatWebIs50530qxd 7/12/05 1142 AM Page 1Using Your Decorating Bag and Coupler1Screw ring off coupler to expose series of tiny2Force coupler base as far down National Centre for Radio Astrophysics. Tata Institute of Fundamental Research. Poonam Chandra. What are Gamma Ray bursts (GRBs)?. Most energetic events in the universe. Long duration GRBs (t>2s) . A . star is a massive ball of plasma that emits . light and electromagnetic energy . throughout the universe. . While . there is only one star in our solar system, there are billions upon billions of stars throughout our galaxy and exponentially more in the billions of galaxies in the universe.