PPT-A Million Second Chandra View of Cassiopeia A

Una Hwang NASAGSFC JHU amp J Martin Laming NRL Boston AAS 24 May 2011 Cas A Firstlight Chandra image Hughes 2000 Red Fe Green Si Cassiopeia A Corecollapse SNR with the most prominent Fe ejecta emission. R Rao 11 K Chandrasekharan 12 Har Gobind Khorana 13 G N Ramachandran 14 Harish Chandra 15 M K Vainu Bappu 16 Postscript 17 Further Reading 18 brPage 2br Cover Page A View of the TIFR Lobby brPage 3br Preface This booklet on some famous scientists o . Statistics. : . 1.8 . Ms. ½. . sq. .deg. . @. 160 . ksec. 1761 . sources. Dec. ’06-June ’07. Catalog. : . Elvis . et. al., . 2009, ApJS 184, 158. Martin Elvis, Francesca . Civano. , . Aldcroft. 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? . Manjil P. Saikia. Department of Mathematical Sciences,. School of Science and Technology,. Tezpur University, India. The Man. and. The Machine. Manjil P. Saikia. 2. Manjil P. Saikia. 3. Chandra can observe X-rays from particles up to the last second before they fall into a black hole!!!. By: Meliha Nesru . January 2, 2012. Cassiopeia was the queen of Ethiopia (Joppa).. The wife of Cephus, the king of Ethiopia.. She had promised peruses to marry Andromeda if he saved her from the monster. . 0. Topic: . Multiwavelength observations. Concepts: . Infrared observations, X-ray observations, Optical observations, EM spectrum . Missions: . “Great Observatories”: . Hubble, Chandra, Spitzer;. Ewan O’Sullivan (SAO). thanks to: J. . Vrtilek. ,. L. David, S. . Giacintucci. , S. . Raychaudhury. , A. . Zezas. ,. . and others. How . i. s the hot Intra-Group Medium formed?. Boston, 20 Nov 2014. K-band. 0.5-2 keV. X-ray Emission Line Spectroscopy of Diffuse Hot Plasma. XMM-Newton RGS. Liu, Wang, Li, & Peterson 2010. Li & Wan 2007. T ~ 3 . x. 10. 6. K . Lx. ~2x10. 38. erg/. s. Chandra ACIS-I. 0. Topic: . Multiwavelength. observations. Concepts: . Infrared observations, X-ray observations, Optical observations, EM spectrum . Missions: . “Great Observatories”: . Hubble, Chandra, Spitzer;. By: . Meliha. . Nesru. . May. 5, . 2012. Cassiopeia was the queen of Ethiopia (Joppa).. The wife of Cephus, the king of Ethiopia.. She had promised peruses to marry Andromeda if he saved her from the monster. . Progenitors and Explosions of Type . Ia. Supernovae. Keiichi Maeda (Kyoto U.). Progenitors – which or even something else?. Double Degenerate (DD. ). WD + WD. Single Degenerate (SD. ). WD + MS/RG. SN2014J. R. Margutti. Harvard . nothing. Margutti 13, 14; . Kamble. 13; . Soderberg. 06, 10. Energy partitioning. SNe. are an OPTICAL . phenomenon. 10. 51. erg. OPTICAL. 10. 47. erg. X-rays/Radio. (17 Years of SN 1987A with Chandra). David Burrows and Kari A. Frank. FOE51 Corvallis June 6, 2017. Built on the work of. PSU Chandra observations:. David Burrows. Sangwook. Park. Judith . National Centre for Radio Astrophysics. Tata Institute of Fundamental Research. Poonam Chandra. What are Gamma Ray bursts (GRBs)?. Most energetic events in the universe. Long duration GRBs (t>2s) .