Magnetars
Magnetars were originally observed as high-energy emitters as either soft gamma-ray repeaters (SGRs) or anomalous x-ray pulsars (AXPs). They are very active, mainly observed as x-ray sources, apparently very young and probably part of the general population of pulsars but with much larger magnetic f...
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creator | Lyne, Andrew |
description | Magnetars were originally observed as high-energy emitters as either soft gamma-ray repeaters (SGRs) or anomalous x-ray pulsars (AXPs). They are very active, mainly observed as x-ray sources, apparently very young and probably part of the general population of pulsars but with much larger magnetic fields. The origin of the large magnetic fields is unclear. |
doi_str_mv | 10.1017/9781108861656.014 |
format | Book Chapter |
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identifier | ISBN: 9781108495226 |
ispartof | Pulsar Astronomy, 2022, p.181-191 |
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language | eng |
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source | Ebook Central Perpetual and DDA |
title | Magnetars |
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