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 ...
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 ...
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 ...
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 ...
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 ...
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 ...
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 ...
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
RAMAN RESEARCH INSTITUTE Other titles: Arial Monotype Corsiva Wingdings Times New Roman StarSymbol Comic Sans MS Default Design X-ray polarisation: ...
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 ...
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 ...
J. Garrett Jernigan. MIT. George R. Ricker (PI) Geoffrey Crew ... Gilbert Vedrenne. Jean-Francois Olive. Michel Boer. UChicago. Donald Q. Lamb. Carlo Graziani ...
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 ...
INPE Advanced Course on Compact Objects Course IV: Accretion Processes in Neutron Stars & Black Holes Ron Remillard Kavli Center for Astrophysics and Space Research
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 ...
... SN1987a_debris_evolution_animation.gif Type II Supernova remnants of different ages Cassiopeia A 300 years old Crab Nebula 1,000 years old Supernova Several ...
UHECRs: AGNs or Spiral galaxies?... or Ellipticals? with Ghirlanda, Tavecchio, Fraternali, Pareschi MNRAS, 390, L88 Can we discriminate between AGN and spirals?
Niels Bohr CompSchool Compact Objects Neutron Star Observables, Masses, Radii and Magnetic Fields Feryal Ozel University of Arizona Lecture 1: Surfaces of Neutron Stars
You are listening to a radio recording of a pulsar (the Vela pulsar) of mass ... parameters have been obtained; precession due to relativistic spin-orbit ...
Science (in press) astro-ph/0709.4301. Talk Outline. Dispersion by the ... A dedicated search. Green Bank Extragalactic Radio Transient Experiment (GERTIE) ...
Title: Slide 1 Last modified by: Kent Morrison Document presentation format: Custom Other titles: Times New Roman Times StarSymbol Arial Symbol Helmet StarBats ...
High Energy Neutrinos via Heavy-Meson Synchrotron Emission in Strong Magnetic Fields ... Signature of Neutrinos from Meson Synchrotron Emission. 16. Event Rate ...
... Proceedings of the 30th International Cosmic Ray ... 1 LORD Lunar Orbital Radio Detector 16 Detection of Ultrahigh-Energy Cosmic Rays and Neutrinos ...
3. Survey of X-ray Pulsars ... An unprecedently deep X-ray pulsar survey will likely compensate observational ... Sky for Unknown Pulsars or Bursting events ...