PPT-Bright but slow – Type II supernovae from OGLE-IV & m

Author : tatiana-dople | Published Date : 2017-05-24

Talk by John McCann Paper by D Poznanski Z KostrzewaRutkowska L Wyrzykowski amp N Blagorodnova OGLEIV OGLE Optical Gravitational Lensing Experiment Phase four

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Bright but slow – Type II supernovae from OGLE-IV & m: Transcript


Talk by John McCann Paper by D Poznanski Z KostrzewaRutkowska L Wyrzykowski amp N Blagorodnova OGLEIV OGLE Optical Gravitational Lensing Experiment Phase four Las . ace decdadcd good pe ni worthes, but mon ycan not moue, I keepe a fayer, but 8 good pe ni worthes but mon ycan not moue, Ikeepe a fayer but good pe ni worthes, but mon ycan not moue, Ikeep a fayer, bu Supernovae . J081659.74+511233.7 . and . J07285387+3349106. . with . the BSU . Observatory. Benjamin . Lombard and Sarah Peck . (Mentor: Professor Jamie Kern). Bridgewater State University. Abstract. Ia. supernova progenitors?. Theory and Observational Signatures. A tale in two parts: Rosanne Di Stefano and . Jeno. . Sokoloski. "Over the state it appears, it presages military action, death and countrywide famine so that the population must seek refuge from their homes.” (1006). Ngaire. . Kerse. , Simon . Moyes. , Chris McLean, Kathy . Peri. , Martin Connolly, Michal . Boyd.. . Background. . Ageing demographic. Tip of the iceberg – prevention. Is there anything under there. Futures Scholarship Program and . Florida . PrePaid. College Plan. (. 2016-17). Florida Bright Futures Scholarship Program. The Florida Bright Futures Scholarship Program rewards students for their academic achievements by providing funding to attend postsecondary institutions in Florida. Circumbinary. . Planet found by Gravitational Microlensing. David Bennett. NASA Goddard. in . collaboration with. . MicroFUN. M. icrolensing . F. ollow-. U. p . N. etwork. OGLE-2007-BLG-349 Binary Lens Model. Y. K. Jung. OGLE, MOA, . KMTNet. collaborations. What We did. Analyze two microlensing events. OGLE-2016-BLG-0733. OGLE-2016-BLG-1003. OGLE-2016-BLG-0733. Deviate . from the symmetric form of an event produced by a single . Array for Sub-. F. ermi . E. nergy . H. eavy Ion . R. eaction . D. ynamics. Summer REU Program 2012. Brittany Abromeit. August 3, 2012. 1. Outline:. Supernovae and the resulting neutron stars. Nuclear Equation of State. Developed by . the SOFIA Team. 0. Topic: . Supernovae. Concepts: . Supernovae, planet formation, infrared observations. Mission: . SOFIA. Coordinated by: . the NASA Astrophysics Forum. An Instructor’s Guide for using the slide sets is available at the ASP website . Favorite web sites. About me. Friends and family. Ogle, 2015. About Me. Freshman. Business management. I grew up in a small town in southwestern Wyoming called Kemmerer. I would love to move to a big city after graduating college to get the “city life” experience. I want to open a bakery/restaurant. I love spending time with my family. They are the world to me. They made me who I am!. 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.. 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. Chelsea Braun. Credit: Artist illustration ESO, http. ://www.universetoday.com/wp-content/uploads/2006/12/2006-1130supernova.jpg. Overview. What is a Supernova?. Types of Supernovae. Supernovae in NGC 4088. Lecture 1. Josh . Frieman. I Jayme . Tiomno. School of Cosmology, Rio de Janeiro, Brazil. July 2010. Hoje. I. Cosmology Review. II. Observables: Age, Distances. III. Type . Ia. Supernovae as . Standardizable.

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