PPT-X-ray Diagnostics and Their Relationship to Magnetic Fields

David Cohen Swarthmore College If we understand the physical connection between magnetic fields in massive stars and Xrays we could use Xray observations to identify magnetic massive stars eg Which of the stars in this Chandra Xray image of the Orion Nebula Cluster are massive magnetic stars . 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’ . 2012. Why and How . Validation of the Coatings with Beams. 2 types of Coatings to be validated: . Magnetron and Hollow Cathode. 2 configurations of magnets pipes:. MBA, MBB. QD and QF as a second priority. David Cohen. Swarthmore College. If we understand the physical connection between magnetic fields in massive stars and X-rays, we could use X-ray observations to identify magnetic massive stars.. e.g. Which of the stars in this Chandra X-ray image of the Orion Nebula Cluster are massive magnetic stars? . at . . EUROTAPE B.V. . Shlomi Bitterman – CEO. May 2011. CIET BIO Diagnostics Ltd.. Area. : . 20,770 sq km. . (The Netherlands = 41,543sq km). Population. : . Christopher F. . McKee. MFU V Corsica. Oct 7, 2015. With: Pak-. Shing. Li. Richard Klein. IN STAR FORMATION. Partial support provided by the National Science Foundation and NASA. OUTLINE. III. Observing interstellar magnetic fields on a computer (LMK). David Cohen. Swarthmore College. X-rays in massive stars are associated with their radiation-driven . winds. Power in these winds: . erg s. -1. . while the x-ray luminosity. To account for the x-rays, only . a physical perspective . . 1. Philip Judge, . . High Altitude Observatory, NCAR. "Double, double, toil and trouble;. Fire burn, and cauldron bubble!". -- . Name . Title. Microsoft Corporation. Agenda. Windows Azure Diagnostics for . Application . Monitoring. Windows Azure PowerShell Cmdlets . for . Diagnostics . Configuring and Analyzing Diagnostic Data . a. nd . Synchrotron . Emission. Dongsu. . Ryu. (CNU), . Magnetism Team . in Korea. Magnetic fields in the intergalactic space. c. lusters of. galaxies:. B ~ a few . m. G. filaments of. galaxies:. at HIMAC synchrotron. Hiroshi Uchiyama . #,A). , Masahiro Kawashima . A). , . Shunsuke. Saito . A). , Izumi Kobayashi . A). , . Tadahiro. . Shiraishi. . A). ,. Chihiro. Kobayashi . A). , Eiichi . Crane Video. What do you know about magnetism?. Electricity and magnetism are related!. Modeling .  independent work  compare notes. Magnetism Readings. Turn and talk. …Partner closer to the door. Consider the following example:. 1) The electron beam is produced by accelerating electrons through an electric potential difference of 380 V. What is the speed of the electrons as they leave the 380 V plate?. The Magnetic Origin of Black Hole Accretion Disk Winds Chris Shrader* (NASA Goddard Space Flight Center ) Collaborators: D. Kazanas (GSFC), K. Fukumura (JMU), F. Tombesi (UMD), Ehud Behar ( The Magnetic Origin of Black Hole Accretion Disk Winds Chris Shrader* (NASA Goddard Space Flight Center ) Collaborators: D. Kazanas (GSFC), K. Fukumura (JMU), F. Tombesi (UMD), Ehud Behar (