Magnetars
نویسندگان
چکیده
منابع مشابه
Timing Properties of Magnetars
We study the pulse morphologies and pulse amplitudes of thermally emitting neutron stars with ultrastrong magnetic fields. The beaming of the radiation emerging from a magnetar was recently shown to be predominantly non-radial, with a small pencil and a broad fan component. We show that the combination of this radiation pattern with the effects of strong lensing in the gravitational field of th...
متن کاملPulsar Physics without Magnetars
Almost 40 years after the discovery of pulsars – and despite a plethora of secured data on them – pul-sar theory is still beset by a number of fundamental inconsistencies. In this short contribution, I will argue that (i) magnetars do not exist, (ii) (ordinary) pulsars turnoff (or 'die') when their wind pressure falls short of keeping the CSM at a safe distance, exceeding 10 15 cm, whereupon th...
متن کاملCoherent Emission from Magnetars
It is proposed that magnetospheric currents above the surfaces of magnetars radiate coherent emission in analogy to pulsars. Scaling the magnetospheric parameters suggests that the coherent emission from magnetars would emerge in the infra-red or optical. Pulsar radio emission and molecular masers are two examples of naturally occurring coherent emission. But there is no accepted analogue in th...
متن کاملThe Birthrate of Magnetars
Magnetars, neutron stars with ultra strong magnetic fields (B ∼ 10−10G), manifest their exotic nature in the form of soft gamma-ray repeaters and anomalous X-ray pulsars. This study estimates the birthrate of magnetars to be ∼ 0.22 per century with a galactic population comprising of ∼17 objects. A population synthesis was carried out based on the five anomalous X-ray pulsars detected in the RO...
متن کاملAlfvén QPOs in Magnetars
We investigate torsional Alfvén oscillations of relativistic stars with a global dipole magnetic field, via two-dimensional numerical simulations. We find that a) there exist two families of quasi-periodic oscillations (QPOs) with harmonics at integer multiples of the fundamental frequency, b) the lower-frequency QPO is related to the region of closed field lines, near the equator, while the hi...
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ژورنال
عنوان ژورنال: Proceedings of the National Academy of Sciences
سال: 1999
ISSN: 0027-8424,1091-6490
DOI: 10.1073/pnas.96.10.5351