Hard X-ray emission from AXPs 1E 1841-045 and 1RXS J 170849.0-40091: ... XMM-Newton. 2) Total. 1E 1841-045; Chandra (Morii et al. 2003) 3) Pulsed. 1E 1841-045; ...
Magnetars: SGRs and AXPs Magnetars in the Galaxy ~7 SGRs, ~12 AXPs, plus candidates, plus radio pulsars with high magnetic fields (about them see arXiv: 1010.4592)
Magnetars: SGRs and AXPs Magnetars in the Galaxy ~11 SGRs, ~12 AXPs, plus candidates, plus radio pulsars with high magnetic fields (about them see arXiv: 1010.4592)
Lecture 4. Magnetars: SGRs and AXPs Sergei Popov (SAI MSU) Magnetars on the Galaxy 5 SGRs, 10 AXPs, plus candidates, plus radio pulsars with high magnetic fields
Approved RXTE observation to search for possible X-ray Pulsar. 0142. 0147 ... Steady spin-down like radio pulsars. Magnetars, dipole spin-down B fields 1014 1015 G ...
Observational Perspective. Simon Johnston. Australia Telescope National Facility. CSIRO ... A whole zoo of new and interesting objects. Magnetars. AXPs / SGRs ...
... points introduced by vacuum effects fall near the line energy and in the ... definite confirmation of their magnetar nature, but also an independent measure ...
Title: Slide 1 Author: Simon Brown Last modified by: sz Document presentation format: On-screen Show (4:3) Other titles: Arial Times New Roman Wingdings Comic Sans MS ...
Glitches; the Link Between the Typical Radio Pulsars and the Anomalous X-ray Pulsars ... Theoretical models for pulsar glitches; star quake and vortex creep ...
typical rotation periods: 1.5 ms 5 s ... I O2 = 3 1052 P-2(ms) erg ... Anti Coincidence Shield (ACS) (512 kg, 91 BGO blocks) The ACS is also used as an ...
Glitches and precession What is a glitch? Crab glitch and the general idea Glitches Phenomenology and the Vela pulsar General features of the glitch mechanism KERS ...
Pulsar research at soft g-rays Lucien Kuiper, Wim Hermsen Hans Bloemen s Outline of presentation Introduction: pulsars in a nutshell Overview current high-energy ...
Neutron stars have been predicted in 30s: L.D. Landau: Star-nuclei (1932) anecdote ... (Landau) (Baade) (Zwicky) 4. Good old classics. The pulsar in the Crab ...
Recent data Calvera et al. LOFAR Gravitational waves from INSs Recent LIGO results for PSRs GWs from young magnetars Detectability by advanced LIGO Magnetar ...
about 65% of HMXBs in the third IBIS cat are SGXBs with massive supergiant early ... IBIS significance image (17-30 keV, 2,000 s exposure ) of the transient IGR ...
Evolution of isolated neutron stars: young coolers and old accretors Sergei Popov (SAI) Plan of the talk Magnetic rotator Evolution of neutron stars: rotation ...
Title: Close-by young isolated neutron stars (and black holes) Author: polar Last modified by: sergepolar Created Date: 4/1/2005 6:24:30 AM Document presentation format
Isolated Neutron Stars. Intro. Stars in the Galaxy Prediction ... Good old classics The old zoo of neutron stars Rocket experiments Sco X-1 UHURU Accretion in close ...
... Proceedings of the 30th International Cosmic Ray ... 1 LORD Lunar Orbital Radio Detector 16 Detection of Ultrahigh-Energy Cosmic Rays and Neutrinos ...
Title: Neutron star masses: dwarfs, giants and neighbors Author: PKSternberg Last modified by: sternberg pk Created Date: 11/26/2005 8:18:07 AM Document presentation ...
pulsar planetary system first discovered in 1992 - and to date the lowest mass planet ... are such disks suitable for planet formation? disks or rings? ...
... been tortured and killed for peacefully protesting. INTRODUCTION ... appropriateness of public police educational programs to respond to the protesting public. ...
However, simply ensuring a signal that agrees with the data also causes fitting to the noise. ... hRSS is strain root sum of squares and is defined as: S( h i ...
Lorimer & Kramer 2005 'Handbook of Pulsar Astronomy' Books. Review Articles ... Lorimer 2005: Binary and MS pulsars. Will, 2006: GR theory and experiment ...
The RIDGE pipeline as a method to search for gravitational waves associated with magnetar bursts LIGO-G080247-00-Z Jason Lee, Tiffany Summerscales (Andrews University) ;
Yosi Gelfand, Greg Taylor, Chryssa Kouveliotou, David Eichler, Yoni Granot, Enrico Ramirez-Ruiz, ... Swift out to 70 Mpc, tail to 10 Mpc - 1% - 20% of short ...
Roche lobe overflow by a secondary without a common envelope. Roche lobe overflow by a secondary with a common envelope. Popov, Prokhorov astro-ph/0505406 ...
HIGH-QUALITY FAST QPOs FROM MAGNETARS: AN ELECTRIC CIRCUIT MODEL A.Stepanov (Pulkovo Observatory, St.Petersburg) V.Zaitsev (Institute of Applied Physics, N.Novgorod)
Isolated Neutron Stars and Black Holes. Intro. Sergei Popov (SAI MSU) Plan Part 1. Neutron stars Prediction ... Good old classics The old zoo of neutron stars Rocket ...
Close-by young isolated neutron stars (and black holes) Sergey Popov (Sternberg Astronomical Institute) Plan of the talk NS: introduction Close-by NSs Population ...
Relation of Electron Fermi Energy With Magnetic Field in Magnetars and their x-ray Luminosity Qiu-he Peng (Nanjing University ) Some published relative works Behavior ...
'Mediante el baloncesto, y en Bilbao, ayudar a ni os, de clases desfavorecidas en ... dar a conocer el baloncesto. aportar medios, humanos y materiales ...
Astrophysical Exotica: degenerate stars with ultrahigh magnetic fields (white ... Pmag=3x1027 dynes/cm (1022 times larger than Pgas in solar photosphere) ...
Evolution with decaying and re ... A model based on field-dependent decay of the magnetic moment of NSs can provide an evolutionary ... Initially the toroidal field ...
Close-by young isolated NSs: A new test for cooling curves Sergei Popov (Sternberg Astronomical Institute) Co-authors: H.Grigorian, R. Turolla, D. Blaschke
Strongest man-made B 107. Radio Pulsars 1012-1013. Magnetars 1014-1015 ... excess from Virgo cluster indicates that at most 5% of short GRBs are SGR GFs or ...