PPT-Supernova Remnants in the ChASeM33 X-ray Survey of M33

Knox S Long William P Blair P Frank Winkler and the ChASeM33 team Abstract M33 contains many emission nebulae identified as supernova remnants SNRs based on the high S IIH alpha ratios characteristic of shocked gas Using Chandra data from the ChASeM33 survey with a 0352 keV sensitivity of about 2 10. Session Objectives. During this session you will learn the following items:. What is STEM?. What is the BSA response?. What are “Counselors” and “Mentors”?. How will the Old North State Council become “STEM-focused”?. Xia Fang. Problems. Thanks for your time. Jim Kneller. NC State University. NOW 2010. The neutrinos we will detect from the next SN in our Galaxy will tell us much about the explosion . and. the neutrino.. The flavour content of the signal changes as it propagates from the proto-neutron star to our detectors here on Earth.. (Supernova Impostors) Schuyler Van Dyk IPAC/Caltech USA Supernova Impostors • Observed outburst with ~10 49 - 50 erg, i.e., comparable to that of a SN • Many impostors spectroscopica Original source: Arnett. , W.D.; et al. (1989). "Supernova 1987A". . Annual Review of Astronomy and Astrophysics. . 27. : 629–700. .. From Wikipedia article, downloaded 9/8/14, . http. ://. en.wikipedia.org/wiki/SN_1987A. Estimates by C. Baltay. DRM 1 compared to IDRM. M. ain . differences as far as Supernovae are concerned:. Larger area Imager. Longer wavelength limit (2.5 microns . vs. 2.0). DRM 1 has same . dia. mirror (1.3 m), DRM 1a has 1.2 m mirror. All that is left. USFWS GRANT. http://www.fws.gov/birdhabitat/Grants/NAWCA/Standard/US/2013_Sept.shtm. This website will take you to the page that announces the 2014 awards for wildlife habitat grants given by the United States Fish and Wildlife Service. . Physics Opportunities with. Supernova Neutrinos. Georg Raffelt, Max-Planck-Institut für Physik, München. Sanduleak -69 202. Sanduleak . -. 69 202. Large Magellanic Cloud . Distance 50 kpc . (160.000 light years). 1. John Beacom, The Ohio State University. 2. Plan of the Talk. Introduction to Supernova . N. eutrinos. Focus on . B. urst . D. etection. . What will we know after the next burst?. What . new capabilities do we need?. Arunas Janusonis. CONTENT. FACTORS OF CONTAMINATION. ASSOCIATION „REMNANTS OF WAR T. H. REAT PREVENTION“. MISSION. PURPOSES. SERVICES. COOPERATION. IMPLEMENTED . PROJECTS. CONTACTS. FACTORS OF CONTAMINATION. N. eutron . Stars Foreseen. . Supernova . End Products?. When a . supernova. goes off, we can speculate that:. The star might blow itself to smithereens, . scattering all its material into space and leaving . Mysterious explosions in the Universe. Poonam Chandra. Royal Military College of Canada. Universe is 14 billion years old.. Our sun is 5 billion years.. Supernovae and Gamma ray bursts. Explosions lasting fraction of a second to few seconds.. biodistribution. and resistance selection. Alessandro . Pini. pinia@unisi.it. Department of Medical Biotechnology. University of Siena. Italy. SetLance srl. Toscana Life Sciences. Italy. The new AMP M33. molecular. . clouds. Armand Fiasson. LAPP - . Annecy-le-vieux. Where. . CRs. . originate. ?. The . usual. suspects up to the . knee. are . s. upernova . remnants. (. SNRs. ). Diffusive . shock.