PPT-The Radio Evolution of the Galactic Center

Magnetar Joseph Gelfand NYUAD CCPP Scott Ransom NRAO Chryssa Kouveliotou GWU Mallory SE Roberts NYUAD Hind Al Ali NYUAD Yoni Granot 2015 December 17 1 28th Texas Symposium on Relativistic Astrophysics. Energy . Q. uantiles. Jaesub Hong. Spring, 2011. Outline. The X-ray sources in the Galactic Bulge. Quantile. Analysis. Periodic. Bulge X. -ray . Sources and Modulating Energy . Quantiles. Galactic Center Region (32’ . Paul Alexander. University of Cambridge. Radio-mode Feedback. Fanaroff & Riley Class-I . 3C . 66B. Fanaroff & Riley Class-II . 3C 219. AGN Feedback via radio sources critical for evolution of massive galaxies. Dan Hooper . - . Fermilab. /University of Chicago University of Michigan Dark Matter Workshop, April . 1. 5. . th. , 2013. Dark Matter in The Galactic Center. The volume surrounding the Galactic Center is complex; backgrounds present are not necessarily well understood . Formation and cosmic evolution of massive black holes. Andrea Merloni. MPE, Garching. Syllabus. Monday:. Observational evidence of Supermassive Black Holes. AGN surveys. Tuesday: . The evolution of SMBH mass function and spin distributions. a prospect from galaxy evolution. Cosmic Microwave Background Radiation and Its Foreground Interstellar Components, Tokyo. , . 17. th. February, 2010. Tsutomu T. TAKEUCHI. Institute for Advanced Research, Nagoya University, Japan. e. arly type galaxies. and their dark matter haloes. Gian. Luigi . Granato. . INAF – Trieste. Cinthia. . Ragone. -Figueroa. Mario . Abadi. IATE-Cordoba. Plan:. Generalities on the problem. Why puffing-up cannot explain what we see so far. INTRODUCTION Optical Counterparts Radio Source Properties Radio Spectra Energy Considerations LOW-LUMINOSITY SOURCES Spiral, Seyfert, and Irregular Galaxies Elliptical Galaxies COMPACT SOURCES Self-Ab Energy . Q. uantiles. Jaesub Hong. Spring, 2011. Outline. The X-ray sources in the Galactic Bulge. Quantile. Analysis. Periodic. Bulge X. -ray . Sources and Modulating Energy . Quantiles. Galactic Center Region (32’ . 23.1 Our Parent Galaxy. 23.2 Measuring the Milky Way. Early “Computers”. 23.3 Galactic Structure. 23.4 The Formation of the Milky Way. 23.5 Galactic Spiral Arms. Density Waves. 23.6 The Mass of the Milky Way Galaxy. . Snežana Stanimirović (UW-Madison). At the end of “GoldenEye”. James Bond goes to Puerto Rico . searching for a gigantic . satellite dish…. “GoldenEye” (1995):. the 17th James . Bond movie. Chapter . 13, . Sections . 1. -5,7 (12 . pages). Homework for Next Time: . www.galaxyzoo.org. Question. Which of these is a picture of the Milky Way?. A. B. D. C. The Milky Way. Angular Size. Andromeda: MW’s Sister Galaxy. Extragalactic radio . s. ources and their importance for astronomy. Leiden 10-13 June 2013. Ron Ekers. CSIRO, . Australia. George Miley. The largest, the furthest, the most powerful, and to some of us the most fascinating objects known in the Universe are to be found among the radio sources associated with some elliptical galaxies and QSO’s. In recent years it has become apparent that they are also objects of considerable beauty.. engineering 1011 and in some key aspts is analogto natural elution In particular this paper details an unconstrained intrinsic HE experiment where a network of transistors sensed and ulised the radio Rachel Osten (. STScI. , JHU). Also . thanksk. to Gregg . Hallinan (. CalTech. ), Laura . Chomiuk. (MSU), . Shami. Chatterjee (Cornell), Joe Lazio (JPL), Tom . Maccarone. (TTU). Outline. Fundamental role of radio observations in transient follow-up; recent JVLA results, motivation for future Brave New Transient World.