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Yiju WON MY HEART Words by Music by FRED STRASSER I Honey honey listen to my plea I fear there146s somethingwrongwith me Now I have your picture on the wall But that don146t help me dear at all. .. " . Predicting the future is much too easy... You look at the people around you, the street you stand on, the visible air you breathe, and predict more of the same. To hell with more. I want better." . 84 . Hiroshi Nagai. (National Astronomical Observatory of Japan). In collaboration with. Monica . Orienti. , Motoki Kino, Kenta Suzuki, Keiichi Asada, Akihiro . Doi. , Gabriele . Giovannini. , Marcello . 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? . Andrew Levan. University of Warwick. Parameter space. Kouveliotou. et al. 1993. Parameter space. Kulkarni. & . Kasliwal. 2010. Parameter space. LGRBs. SGRBs. SGRs. ?. TDEs?. Galactic sources (SGR, LMXB, HMXB, . X-Ray Diffraction. I. X-Ray Diffraction. Uses X-Rays to identify the arrangement of atoms, molecules, or ions within a crystalline solid. Quantitative and qualitative . Ooi. , L. . Principles of X-ray Crystallography . Guanghui Zhu. Instrument Report:. Contents. Diffraction Mechanism. C. onstruction . of . the . Diffractometer. Applications . of . XRD. Data . A. nalysis . and . Explanation. 2D XRD. XRD Simulation. Diffraction . R. N. Manchester. CSIRO Astronomy and Space Science Australia . Telescope National Facility. , Sydney. Summary. Pulse profiles – doubles and . interpulses. High . Edot. pulsars – radio and high-energy emission. . Wei Wang. National Astronomical Observatories, . B. eijing China. The IAU XXVII General Assembly, Beijing August 20-31 2012. IAUS 291 . Neutron stars and pulsars: Challenges and opportunities after 80 Years. and Other Applications: Hydrology +. Neutron Monitor Community Workshop—Honolulu, Hawaii . October . 24-25, 2015. Physicist. National Urban Security Technology Laboratory . Science and Technology Directorate. Centaurus. X-3 Over its Binary Orbit”. -. Sachindra. Naik, . Biswajit. Paul, and . Zulfikar. Ali. Introduction:. Interest: Extended dips in the light curve. Cen-X: Eclipsing HMXRB pulsar. Orbital period ~2.1 days, pulse period ~4.8 s. thermal components. Rhaana. Starling. University of Leicester. Royal Society Dorothy Hodgkin Fellow. With special thanks to Martin . Sparre. (. DARK/Leicester) . and Kim Page (Leicester). Outline. GRB X-ray spectra – the basic shape. . for . bioinformatics . Robbie P. Joosten. Netherlands Cancer Institute. Autumnschool. 2013. S. tructures . in . bioinformatics. Understand biology. Direct . interpretation. Data mining. Homology . Visible structures. 1.  - Trachea. 2.  - Hila. 3.  - Lungs. 4.  - Diaphragm. 5.  - Heart. 6.  - Aortic knuckle. 7.  - Ribs. 8.  - Scapulae. 9.  - Breasts. 10.  - Bowel gas. Normal chest X-ray anatomy. some views on its status. and perspectives. September. , 15th 2021. . P. hilippe Laurent. CEA/DRF/IRFU/. DAp. Gamma-ray astronomy status and perspective. Plan. Current/future hard X-ray/. -ray. telescopes.