Friday, October 15, 2010

A Low-Magnetic-Field SGR

Rea et al. present the discovery of an SGR with a weak dipole field.  This object emits bursts, has a strong persistent x-ray emission (i.e. it is hot) and exhibits pulsed profile changes -- it acts like a magnetar.   The discovery points out what has been known unconsciously for a long time that the location of a pulsar on the P-Pdot diagram has little to do with its surface and internal fields.   Rea et al. argue that this could mean that any pulsar could turn into a magnetar whenever.  I think that this is a bit of a reach because we also think that magnetars are typically young as demonstrated by their association with supernova remnants and OB associations. Pretty Neat!

arXiv:1010.2781 [pdfotherTitle: A low-magnetic-field Soft Gamma Repeater

2 comments:

sgd said...

if "the location of a pulsar on the P-Pdot diagram has little to do with its surface and internal fields", why all the "magnetars" are in the same region of the P-Pdot diagram??? ;) Pretty Neat!

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