PPT-The Galactic Interstellar Halo

Suggested Reading Hot halo via Xray lines http adsabsharvardedu abs2012ApJ756L8G httpsarxivorgpdf12113137pdf Diskhalo via optical amp UV lines httpadsabsharvardeduabs2012ARA26A50491P. 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. Not as Empty as You Might Think. Dr. Andrew Fox. Space Telescope Science Institute/European Space Agency . Hubble Science Briefing. April 5 2012. What is a galaxy made of?. 2. 2. Stars. Dark Matter. Interstellar Gas & Dust. 5. th. Feb 2015. Introducing HALO. Contents. Halo – Rapid Deployment Demonstration Kit. Easy to Transport : . HALO RDD Kit is easy to transport – comes packed in a . pelicase. for easy transport. Philip Lubin. Physics Dept – UC Santa Barbara. lubin@deepspace.ucsb.edu. http://arxiv.org/abs/1604.01356. NASA 360 Video – “Going Interstellar” . . www.facebook.com/FollowNASA360/videos. www.youtube.com/user/FollowNASA360. Part II: Interstellar . Gas. . . Gas . Absorbing. Light. In addition to dust grains, there is low-density gas between the stars. . This leads to the formation of . additional . absorption . lines in the spectrum of a star. Twinkle, twinkle, little star, how I wonder what you are?. What are stars?. And what are they made of?. Stars are huge, hot, bright balls of gas.. Stars have different temperatures.. Stars are of different colors.. . 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. Ralf Herbrich. Applied Games Group. Microsoft Research Cambridge. Microsoft Research. 1991. 1997. 1998. 2001. 2005. 2008. Overview. Why Machine Learning and Games?. Machine Learning in Video Games. Drivatars. Hao. Zhang. University of Maryland/University of Liverpool/Cockcroft Institute. Outline. Introduction. Motivation to Study Beam Halo. Method. Adaptive Method Using Digital Micro-mirror Device. Experiment . An X-ray/UV Perspective. Edmund Hodges-. Kluck. Joel . Bregman. . University of Michigan. How do baryons cycle in and out of galaxies, and how does this impact galaxy evolution?. What happened to the “missing” baryons?. Lerman Non-Invasive Halo ( NIH ). . Designed to address and overcome to complications associated with the use of the Traditional Invasive Halo. . Lerman NIH. Padded carbon composite. Lerman Non-Invasive Halo ( NIH ). . Designed to address and overcome to complications associated with the use of the Traditional Invasive Halo. . Lerman NIH. Padded carbon composite. Nicholas Fantin. NGVS Meeting, . September 22. nd. , 2016. Outline. Motivation. Selecting White Dwarf Candidates. Photometric and Kinematic Properties. Halo White Dwarfs. Next Steps. Summary. Motivation.