By Silvia Zane, Roberto Turolla, Dany Page
This e-book collects the contributions awarded on the convention remoted Neutron Stars: From the skin to the internal, held in London in April 2006. 40 years after the invention of radio pulsars it offers an updated description of the recent imaginative and prescient of remoted neutron stars that has emerged in recent times with the improvement of multi-wavelength observations. the nice number of remoted neutron stars, from pulsars to magnetars, a few of them came upon very lately and plenty of of them now not detectable in radio wavelengths, is abundantly coated by means of descriptions of modern observational effects and shows of the newest theoretical interpretation of those data.
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Additional resources for Isolated Neutron Stars: from the Surface to the Interior (V. 308 No. 1-4)
Bursting activity from SGR 1806–20 resumed at the end of 2003 displaying an increase in both the γ -ray burst rate and the hard X-ray persistent emission (Mereghetti et al. 2005b) throughout 2004, and culminating with the giant flare of 27th December 2004 (Borkowski et al. 2004, during which ∼1047 erg were released for a distance of about 10 kpc; Cameron et al. 2005; McClure-Griffiths and Gaensler 2005). The event was so intense that caused a 26 strong perturbation in the Earth ionosphere and saturated the detectors on every high-energy satellite.
2002, 2003). All 5 detectors of the PCA were operating normally and their photons were co-added. The data were recorded in the event-mode and good Xenon configurations, with 125 µs time resolution and 64 energy channels covering 2–60 keV. We excluded faint bursts that do not have enough counts to accumulate an individual spectrum, and very bright bursts with count rates exceeding 90 000 counts s−1 where deadtime and pileup effects become significant. We classified the bursts according to their light curve morphology into singlepeak and multi-peak bursts and fitted each emission peak separately.
56 s modulation. A similar interpretation was originally proposed by Feroci et al. (2001) (see also Thompson and Duncan 2001) to explain the smooth flux decay in the first tens of seconds of the 1998 giant flare from SGR 1900+14. Indeed, a variety of seismic modes are expected to be excited as consequence of the magneticallyinduced large scale fracturing of the crust which gives rise to giant SGR flares. Astrophys Space Sci (2007) 308: 25–31 Out of the variety of non-radial neutron star modes studied by McDermott et al.