PPT-Study on circumstellar maser sources

and the JVN towards the SKA Hiroshi Imai Research and Education Assembly Science and Engineering Area International Radio Astronomy Collaboration Promotion Office Kagoshima University SiO masers around . McMahon James and J Parnell School of Geosciences University of Aberdeen Aberdeen AB24 3UE UK seanmcmahonabdnacuk School of Physics A tronomy University of St Andrews North Haugh St Andrews Fife KY16 9SS School of Geosciences Univers ty of The study of studying History. Thoughts on History. “The most effective way to destroy people is to deny and obliterate their own understanding of their history.” . ― . George . Orwell. “That men do not learn very much from the lessons of history is the most important of all the lessons that history has to teach.” . Hiroshi Imai. Graduate School of Science and Engineering. Kagoshima University. A Neapolitan of Masers: Variability, Magnetism and VLBI . 20 . May 2013, . CSIRO CASS, . Australia. Water fountain. highly collimated, fast, stellar, molecular jet . NIS . Aktobe. , 2013. Criteria of credibility (RAVEN). Expertise. (does the source have specialised knowledge and does the situation demand it?). Neutrality. (is the source predisposed to support a particular point of view for reasons other than vested interest. Bright young things, lasers and alcohol. Spitzer mid-IR image of the DR21 region in the Cygnus-X molecular complex. Image Credit: . NASA, Spitzer Space Telescope.. Aims of the project. To test our best models of methanol masers. in Maser Theory. Vladimir Strelnitski. Maria Mitchell Observatory. “Radio Stars” . Haystack Observatory. 4 October, 2012. Plan . . 1. Summary of Maser Theory. . - . Uniqueness of Inversion. Hiroshi Imai. Graduate School of Science and Engineering, Kagoshima University. Contents. Astrometry with VLBA. , and VERA (EVN . for OH masers) . Results of astrometry. IRAS 19134+2131. K3-35. IRAS 19312+1950. P. olarization and Magnetic fields during Massive Star Formation. W. H. T. . Vlemmings. ASP Conference Series, Vol. 387, 2008. Do-Young . Byun. Outline. Theoretical . Background. Zeeman Effect. Para- and non-paramagnetic Species. Vladimir Strelnitski. Maria Mitchell Observatory. “Radio Stars” . Haystack Observatory. 4 October, 2012. Plan . . 1. Summary of Maser Theory. . - . Uniqueness of Inversion. . - Pumping Cycles. Chapter 1, Lesson 4. Final Lesson. Objective. To learn what methods historians use to study the past.. What approaches do Historians use to examine past events?. Find patterns in past events. Look for causes and effects that explain how and why events happened. by. James Moran. Harvard-Smithsonian Center for Astrophysics. Lo Memorial Lecture. Xinjiang Astronomical Observatory. September 19, 2018. Kwok-Yung (Fred) Lo. 1947 - 2016. Jan Lo and Susan Moran, January 1983. USING DATA ON EXTRAGALACTIC DIFFUSE . GAMMA-RAY EMISSION. . A. . Uryson. Lebedev. Physical Institute RAS, . Moscow. INTRODUCTION. UHECR data are obtained by Pierre Auger Observatory (PAO) and Telescope Array (TA):. Gabe Maser of Government Relations and National Strategy for the Code Council, where he manages and directs its federal and national policy and legislative priorities agen da, and maintains and How do you evaluate the quality of the courses you took and study material you received at your host institution scale 1-5 1poor/negative 5excellentOther please specify Duration of language training