Magnetars: general properties and recent developments

Warning The system is temporarily closed to updates for reporting purpose.

Göğüş, Ersin (2011) Magnetars: general properties and recent developments. In: Astrophysics of Neutron Stars 2010: A Conference in Honor of M. Ali Alpar, Çeşme, İzmir, Türkiye

Full text not available from this repository.

Official URL: http://dx.doi.org/10.1063/1.3629499


Magnetars, which form a growing subgroup of neutron stars, possess the strongest magnetic field environments in the universe. The last few years has been very fruitful for magnetars: three new sources were discovered and one source was correctly identified as an SGR, and all these sources have been studied in depth across the electromagnetic spectrum. Here, we present a brief overview of the latest developments in the world of magnetars and discuss their implications on the estimates of the number of magnetar sources and the rate at which they might emit extremely energetic giant flares.

Item Type:Papers in Conference Proceedings
Subjects:Q Science > QB Astronomy > QB460-466 Astrophysics
Q Science > QC Physics
ID Code:17387
Deposited By:Ersin Göğüş
Deposited On:16 Nov 2011 11:08
Last Modified:30 Jul 2019 14:22

Repository Staff Only: item control page