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)
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 ...
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 ...
MAGNETARS. Ultra-Strong Magnetic Fields producing Gamma Ray flashes and ... impossible by Magnetic forces which are feeble compared to gravity or pressure. ...
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 ...
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
HIGH-QUALITY FAST QPOs FROM MAGNETARS: AN ELECTRIC CIRCUIT MODEL A.Stepanov (Pulkovo Observatory, St.Petersburg) V.Zaitsev (Institute of Applied Physics, N.Novgorod)
Title: Prezentacja programu PowerPoint Author: Krystyna Wosinska Last modified by: Krystyna Wosi ska Created Date: 11/28/2004 8:37:45 AM Document presentation format
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 ...
HE astrophysicists tell helioseismologists where the flare ... Gallagher, P. personal communication 2004. Stanford, January 27 2005. Archive cartoon from ...
The energy release in a single giant flare is of the order of the total ... Giant flares from extragalactic SGRs might explain short duration GRBs. ...
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 ...
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 ...
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 ...
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) ;
Recent data Calvera et al. LOFAR Gravitational waves from INSs Recent LIGO results for PSRs GWs from young magnetars Detectability by advanced LIGO Magnetar ...
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 ...
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 ...
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 ...
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 ...
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 ...
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 ...
Evolution of isolated neutron stars: young coolers and old accretors Sergei Popov (SAI) Plan of the talk Magnetic rotator Evolution of neutron stars: rotation ...
J. Garrett Jernigan. MIT. George R. Ricker (PI) Geoffrey Crew ... Gilbert Vedrenne. Jean-Francois Olive. Michel Boer. UChicago. Donald Q. Lamb. Carlo Graziani ...
New Views of Compact Object Mergers Via Short Gamma-Ray Bursts ... J. Wren, LANL. B. L. Lee, U. Toronto. P. J. McCarthy, Carnegie. D. C. Murphy, Carnegie ...
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
Isotropic gamma-ray energies range from 1051 to 1054 erg ... THREE INTERESTING GAMMA-RAY BURST/SUPERNOVA PARAMETERS. THE Epeak-Eisotropic energy RELATION ...
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 ...
GRB Gamma Ray Bursts An Ongoing Mystery, Evolving Quickly John G. Learned University of Hawaii with s from many folks, Particularly Kevin Hurley and Guido ...
RAMAN RESEARCH INSTITUTE Other titles: Arial Monotype Corsiva Wingdings Times New Roman StarSymbol Comic Sans MS Default Design X-ray polarisation: ...
UHECRs: AGNs or Spiral galaxies?... or Ellipticals? with Ghirlanda, Tavecchio, Fraternali, Pareschi MNRAS, 390, L88 Can we discriminate between AGN and spirals?