Highly Magnetized Accreting Pulsars: Are There Accreting Magnetars?
2S 0114+650, GX 301-2, IGR J16358-4726, X Per, 4U 2206+54, SXP 1062, and 3A 1954+319 are thought to possess high magnetic elds. They have recently been named accreting magnetars, or highly magnetized accreting pulsars. In this work their properties are reviewed. Within the context of their observati...
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doaj-b7d81dea38ca46639271dead8bb742972020-11-24T23:00:04ZengCTU Central LibraryActa Polytechnica CTU Proceedings2336-53822014-12-011121522110.14311/APP.2014.01.02152202Highly Magnetized Accreting Pulsars: Are There Accreting Magnetars?Pere Blay0Pablo Reig1Víctor Reglero2IPL, University of Valencia, SpainUniversity of Crete, GreeceIPL, University of Valencia, Spain2S 0114+650, GX 301-2, IGR J16358-4726, X Per, 4U 2206+54, SXP 1062, and 3A 1954+319 are thought to possess high magnetic elds. They have recently been named accreting magnetars, or highly magnetized accreting pulsars. In this work their properties are reviewed. Within the context of their observational properties (mainly from INTEGRAL data), and the recent models of accretion onto highly magnetized neutron stars, their similarities and dierences are analyzed. The aim is to find a common framework to understand the evolution (in terms of past and present history) of these sources, and to establish the basis of a possible new kind of accreting sources. Two of these sources, namely X Per and 4U 2206+54, contain a massive main-sequence companion, while the rest are supergiant X-ray binaries or symbiotic systems. The variety of astrophysical scenarios represented by this set is wide, therefore the study of these systems is also important in order to establish commonalities between the dierent types of accreting X-ray pulsars and to study the possible evolutionary links between them.https://ojs.cvut.cz/ojs/index.php/APP/article/view/2390 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Pere Blay Pablo Reig Víctor Reglero |
spellingShingle |
Pere Blay Pablo Reig Víctor Reglero Highly Magnetized Accreting Pulsars: Are There Accreting Magnetars? Acta Polytechnica CTU Proceedings |
author_facet |
Pere Blay Pablo Reig Víctor Reglero |
author_sort |
Pere Blay |
title |
Highly Magnetized Accreting Pulsars: Are There Accreting Magnetars? |
title_short |
Highly Magnetized Accreting Pulsars: Are There Accreting Magnetars? |
title_full |
Highly Magnetized Accreting Pulsars: Are There Accreting Magnetars? |
title_fullStr |
Highly Magnetized Accreting Pulsars: Are There Accreting Magnetars? |
title_full_unstemmed |
Highly Magnetized Accreting Pulsars: Are There Accreting Magnetars? |
title_sort |
highly magnetized accreting pulsars: are there accreting magnetars? |
publisher |
CTU Central Library |
series |
Acta Polytechnica CTU Proceedings |
issn |
2336-5382 |
publishDate |
2014-12-01 |
description |
2S 0114+650, GX 301-2, IGR J16358-4726, X Per, 4U 2206+54, SXP 1062, and 3A 1954+319 are thought to possess high magnetic elds. They have recently been named accreting magnetars, or highly magnetized accreting pulsars. In this work their properties are reviewed. Within the context of their observational properties (mainly from INTEGRAL data), and the recent models of accretion onto highly magnetized neutron stars, their similarities and dierences are analyzed. The aim is to find a common framework to understand the evolution (in terms of past and present history) of these sources, and to establish the basis of a possible new kind of accreting sources. Two of these sources, namely X Per and 4U 2206+54, contain a massive main-sequence companion, while the rest are supergiant X-ray binaries or symbiotic systems. The variety of astrophysical scenarios represented by this set is wide, therefore the study of these systems is also important in order to establish commonalities between the dierent types of accreting X-ray pulsars and to study the possible evolutionary links between them. |
url |
https://ojs.cvut.cz/ojs/index.php/APP/article/view/2390 |
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