PPT-Pulsars

Author : mitsue-stanley | Published Date : 2016-06-24

httpwwwcvnraoeducourseastr534Pulsarshtml httpwwwnikhefnlpubonderzoekschooltopicsKuijpers1pdf High Energy Astrophysics jlcmssluclacuk httpwwwmssluclacuk Enrico Massaro

Presentation Embed Code

Download Presentation

Download Presentation The PPT/PDF document "Pulsars" is the property of its rightful owner. Permission is granted to download and print the materials on this website for personal, non-commercial use only, and to display it on your personal computer provided you do not modify the materials and that you retain all copyright notices contained in the materials. By downloading content from our website, you accept the terms of this agreement.

Pulsars: Transcript

httpwwwcvnraoeducourseastr534Pulsarshtml httpwwwnikhefnlpubonderzoekschooltopicsKuijpers1pdf High Energy Astrophysics jlcmssluclacuk httpwwwmssluclacuk Enrico Massaro notes. . rce m y t han utheg nd arsd heo . The w ati thenart with esteriao lse p Millisecond . Pulsars:. Dan Stinebring. Oberlin College. CWRU – May 21, 2009. . George Greenstein. (Amherst College). Discovery of “Millisecond” Pulsars. 1982 – Arecibo Observatory – Don Backer, Sri Kulkarni, .... NanoHertz. Observatory of Gravitational Waves. Andrea N. Lommen. Chair, . NANOGrav. Associate . Professor of Physics and Astronomy. Head of Astronomy Program. Director of Grundy Observatory. Franklin and Marshall College. Dan Hooper . - . Fermilab. /University of Chicago University of Michigan Dark Matter Workshop, April . 1. 5. . th. , 2013. Dark Matter in The Galactic Center. The volume surrounding the Galactic Center is complex; backgrounds present are not necessarily well understood . 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 . 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. . 22/10/2011 INDIGO . discussions@IUCAA. . Bhal. Chandra Joshi . Radio pulsar searches . Radio pulsars - highly magnetized rotating NS - compact . - periodic pulses . 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 . Sergei Popov. (SAI MSU). Plan. General intro. Pulsar models. Population synthesis. Summary of discoveries. EGRET legacy. Just 6 pulsars:. Crab. Geminga. Vela. PSR B1055-52. PSR B1706-44 . PSR B1951+32 . . 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. 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 . Ingrid Stairs. UBC Vancouver. CAWONAPS. TRIUMF. Dec. 9, . 2010. Pulsars are one manifestation of neutron stars:. spin periods ~. 1.4. ms to . 8.5 seconds,. magnetic fields ~10. 8. to ~5 x10. 13. G. . 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 . known. . pulsars: past searches and future prospects. Matthew . Pitkin (on behalf of the LIGO Scientific Collaboration & Virgo Collaboration). University of . Glasgow. m. atthew.pitkin@glasgow.ac.uk.

Download Document

Here is the link to download the presentation.
"Pulsars"The content belongs to its owner. You may download and print it for personal use, without modification, and keep all copyright notices. By downloading, you agree to these terms.