PPT-Case Solutions and SuperNova

Instrument Chemistries for each step in the decontamination process Precleaning Manual cleaning Automated cleaning Case Solutions CSR Ink and adhesive remover SchmutzOff stainless steel acid based reconditioner and . 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”?. Supernova Remants and Pulsar Wind Nebulae in the Chandra Era. 1. Modeling the Dynamical and Radiative Evolution of a Pulsar Wind Nebula inside a Supernova Remnant. Joseph Gelfand (NYU / NSF). Patrick Slane (CfA), Weiqun Zhang (NYU). (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. 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 . Highlights of the past 25 years. Outstanding mysteries and surprises. What we can expect to learn, sooner and later. TOPICS. Supernova Energy Sources. Core collapse: . with WFIRST . DRM1 and DRM2. C Baltay. June 1, 2012. Supernova Surveys . using . Slitless. Spectroscopy. Use Imager for . SNe. discovery and to get . lightcurves. Use . slitless. spectroscopy to type supernovae and get redshifts. . . . Sumit K. . Sarbadhicary. PITT-PACC, University of Pittsburgh. Team. - . Carles. . Badenes. (Pitt), Laura . Chomiuk. , Daniel Huizenga, Jessica Maldonado (MSU), . Damiano. . Caprioli. (U. Chicago). What is a supernova?. AND NOW. …. A SUPERNOVA IS A STAR THAT INCREASES IN BRIGHTNESS BECAUSE IT’S MASS IS EXPLODING(AWESOME!!!!!!) . HOW . HOT. . IS. . A. . SUPERNOVA. ?. Supernovae can get up to 100 billion degrees Fahrenheit! That is like1 billion suns and possibly more!. supernovae in LIRGs. Image processing courtesy Mischa Schirmer (Gemini Obs.). Supervisors:. . Stuart Ryder. Richard McDermid. Erik Kool. Macquarie University / AAO. Collaborators: . . Seppo Mattila. © 2010 Case Medical, Inc.. Why choose Case Medical’s instrument chemistries?. Super concentrated and ready-to-use cleaners for each step in the decontamination process. Environmentally-friendly with no added dyes, perfumes, fillers or masking agents. Developed by . the SOFIA Team. 0. Topic: . Supernovae.. Concepts: . Supernovae, planet formation, infrared observations. Missionb. : . SOFIA. Coordinated by: . the NASA Astrophysics Forum. An Instructor’s Guide for using the slide sets is available at the ASP website . Most stars either have M < 1.4 . M. ʘ. , . or can lose enough mass during post-main sequence evolution to get there, and end as white dwarf. However if core is more massive, nothing can stop gravitational collapse.