PPT-Astrophysics of the Galactic Center Part I:

Author : mofferro | Published Date : 2020-06-26

Giant Shocks in the Fermi Bubbles and the Origin of the Microwave Haze Roland Crocker ARC Future Fellow Australian National University image credit NASA Geoff Bicknell

Presentation Embed Code

Download Presentation

Download Presentation The PPT/PDF document "Astrophysics of the Galactic Center Part..." is the property of its rightful owner. Permission is granted to download and print the materials on this website for personal, non-commercial use only, and to display it on your personal computer provided you do not modify the materials and that you retain all copyright notices contained in the materials. By downloading content from our website, you accept the terms of this agreement.

Astrophysics of the Galactic Center Part I:: Transcript

Giant Shocks in the Fermi Bubbles and the Origin of the Microwave Haze Roland Crocker ARC Future Fellow Australian National University image credit NASA Geoff Bicknell RSAA Ettore Carretti Cagliari Observatory. Chapter 0, Introduction. Yosuke Mizuno. Institute of Astronomy. National . Tsing-Hua. University. Lecture Website. Lecture Website. http://. www.phys.nthu.edu.tw. /~. mizuno. /. plastro.htm. l. No specific text book for this lecture. Programs in . Research, Analysis and Enabling Technology . J. S. Gallagher. Comments from the Perspective of the Panel Chair. JSG APC 7/13/11. 1. Review of Astrophysics. Programs . in. . Research, Analysis and. 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. Mark Morris. UCLA. ABSTRACT -- The . well-defined, massive disk of young stars orbiting within 0.5 pc of the Galactic black hole (GBH) is strongly tilted with respect to the Galactic plane. In the context of in situ formation mechanisms, this orientation is inherited from that of the gas disk that formed these stars on the order of 6 million years ago. The tilt can be understood by positing that clouds fall toward the GBH on near-zero angular momentum orbits and form dispersion rings as they self-intersect after . sun = with the . Jansky. Very Large Array. Rick . Perley. NRAO -- Socorro. Goals of This Presentation. Introduce the . Jansky. Very Large Array (7 slides). A major upgrade of the VLA. H. ow does a radio interferometer do . Astrophysics ACTIVITIES ASTROPHYSICS MAJORS DO: Astronomy is some�mes considered a sub�eld of physics. Astrophysics is a specializa�on in the �eld of astro S. R. Kulkarni. Supernova . remnan. . The blue emission is X-ray and arises. from relativistic electrons. Red (. Xray. ). Green Forbidden Optical Line. Guitar nebula: Pulsar traveling at 2000 km/s. Charge exchange!. 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. of . Principal . Component Analysis. Zachariah . Schrecengost. 1. , . Shashi. . Kanbur. 1. 1. SUNY. Oswego, Oswego, NY. NSF . Office of International Science and Engineering award number . 1065093. 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. La gamme de thé MORPHEE vise toute générations recherchant le sommeil paisible tant désiré et non procuré par tout types de médicaments. Essentiellement composé de feuille de morphine, ce thé vous assurera d’un rétablissement digne d’un voyage sur . ronomy Astrophysics 586 49 Maurizio . Spurio, . maurizio.spurio@unibo.it. . Università. di Bologna e INFN. 1. M. Spurio - Galactic template neutrino searches. Propagation induces accidents. M. Spurio - Galactic template neutrino searches.

Download Document

Here is the link to download the presentation.
"Astrophysics of the Galactic Center Part I:"The content belongs to its owner. You may download and print it for personal use, without modification, and keep all copyright notices. By downloading, you agree to these terms.