PPT-The Super-slow Pulsation X-ray Pulsars in High Mass X-ray

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Wei Wang National Astronomical Observatories B eijing China The IAU XXVII General Assembly Beijing August 2031 2012 IAUS 291 Neutron stars and pulsars Challenges

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The Super-slow Pulsation X-ray Pulsars in High Mass X-ray: Transcript

Wei Wang National Astronomical Observatories B eijing China The IAU XXVII General Assembly Beijing August 2031 2012 IAUS 291 Neutron stars and pulsars Challenges and opportunities after 80 Years. How I changed my relationship with fashion, moving from an ego-centric position to an eco-centric position.. 2008 . Started to be disenchanted with fashion system.. Too many clothes, too much waste.. Pulsafeeder’s Pulsation Dampeners improve pump system efficiency by removing pulsating flows from positive displacement pumps , i nsuring a smooth and continuous fluid flow and metering accu WANNER Pulsation Dampeners NEW! Pulsation Dampeners Markets Served • Chemical• Pulp,Textile• Gas, • Biotech/Pharmaceutical• Paint• Food• Consumer• WaterTrea Conclusions. Barausse. E., 2012, MNRAS, 423, 2533. De . Rosa G., . Decarli. R., Walter . F.,Fan. X., Jiang L., Kirk J., . Pasquali A., . Rix. H. . W. ., 2011, . ApJ. , 739, 56;. F. an . X., Strauss M.A., Schneider D.P., Becker R.H., White R.L., . High and Ultrahigh . Energy Cosmic Rays. Ke . Fang. University of Chicago. ISCRA . - . Jul 9, . 2012. 1. KF, . Kotera. , . Olinto. 2012, . ApJ. , 750, 118 . KF, . Kotera. , . Olinto. 2012, in prep. Renaissance due to . Fermi. evaporating PSR discoveries. many wind-driving . Fermi. MSP – Roberts ‘11. Clearly, radio selection effect biased previous sample. Radio plane survey P. B. bias to long periods, weak winds. http://www.cv.nrao.edu/course/astr534/Pulsars.html. http://www.nikhef.nl/pub/onderzoekschool/topics/Kuijpers1.pdf. High Energy Astrophysics. jlc@mssl.ucl.ac.uk. http://www.mssl.ucl.ac.uk/. Enrico Massaro notes. 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. The Pulsar Search Collaboratory. Questions We Will Answer. What is a . pulsar. ?. Why do astronomers study pulsars?. What is the . PSC. ?. How can . you. get involved?. What is a pulsar?. A pulsar is a . Enrico Bozzo. University. of Geneva. Transitional pulsars pulsations at unprecedentedly low X-ray Luminosities. XSS 12270-4859. P. spin. = 1.69 ms. L. X. = 5x10. 33. erg/s. (. Papitto. et al. 2015) . David Smith. Centre d’Etudes Nucléaires de Bordeaux-Gradignan. ( CENBG - in2p3 - CNRS ). I. nstitut. de Physique Nucléaire de Lyon. 6 mars 2015. Le ciel en rayons gamma. avec le. . satellite . Fermi . from the ground based and . INTEGRAL. photometry. International meeting on variable stars research KOLOS 2013, December 5 - 7, 2013, . Kolonica. Saddle. 1. . Institute of . Physics. ,. Faculty . of . 20.11. 1. Neutron stars. T. he . remains of cores of some massive stars that have become supernovae. .. Cores are . a degenerate gas of mostly neutrons.. So much compression at each stage of core contraction that final radius is . Jocelyn Bell . Burnell. University of Oxford Astrophysics . And. Mansfield College. 1957. 2. 3. Crab PSR almost discovered I. Late . summer 1957; . an Open Night . at McDonald; . 82 inch . (Struve) telescope .

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