Matches in SemOpenAlex for { <https://semopenalex.org/work/W2144871911> ?p ?o ?g. }
- W2144871911 endingPage "2924" @default.
- W2144871911 startingPage "2910" @default.
- W2144871911 abstract "The origin of the strong magnetic fields measured in magnetars is one of the main uncertainties in the neutron star field. On the other hand, the recent discovery of a large number of such strongly magnetized neutron stars, is calling for more investigation on their formation. The first proposed model for the formation of such strong magnetic fields in magnetars was through alpha-dynamo effects on the rapidly rotating core of a massive star. Other scenarios involve highly magnetic massive progenitors that conserve their strong magnetic moment into the core after the explosion, or a common envelope phase of a massive binary system. In this work, we do a complete re-analysis of the archival X-ray emission of the Supernova Remnants (SNR) surrounding magnetars, and compare our results with all other bright X-ray emitting SNRs, which are associated with Compact Central Objects (CCOs; which are proposed to have magnetar-like B-fields buried in the crust by strong accretion soon after their formation), high-B pulsars and normal pulsars. We find that emission lines in SNRs hosting highly magnetic neutron stars do not differ significantly in elements or ionization state from those observed in other SNRs, neither averaging on the whole remnants, nor studying different parts of their total spatial extent. Furthermore, we find no significant evidence that the total X-ray luminosities of SNRs hosting magnetars, are on average larger than that of typical young X-ray SNRs. Although biased by a small number of objects, we found that for a similar age, there is the same percentage of magnetars showing a detectable SNR than for the normal pulsar population." @default.
- W2144871911 created "2016-06-24" @default.
- W2144871911 creator A5001612320 @default.
- W2144871911 creator A5047522800 @default.
- W2144871911 creator A5049901789 @default.
- W2144871911 creator A5080499359 @default.
- W2144871911 date "2014-09-12" @default.
- W2144871911 modified "2023-10-03" @default.
- W2144871911 title "Comparing supernova remnants around strongly magnetized and canonical pulsars" @default.
- W2144871911 cites W1572187322 @default.
- W2144871911 cites W1621979734 @default.
- W2144871911 cites W1675475973 @default.
- W2144871911 cites W1731602199 @default.
- W2144871911 cites W1757987097 @default.
- W2144871911 cites W1789352290 @default.
- W2144871911 cites W1844043913 @default.
- W2144871911 cites W1856039017 @default.
- W2144871911 cites W1859783476 @default.
- W2144871911 cites W1968801628 @default.
- W2144871911 cites W1970873592 @default.
- W2144871911 cites W1974254363 @default.
- W2144871911 cites W1977154777 @default.
- W2144871911 cites W1978615856 @default.
- W2144871911 cites W1979941495 @default.
- W2144871911 cites W1980224506 @default.
- W2144871911 cites W1980396493 @default.
- W2144871911 cites W1980998756 @default.
- W2144871911 cites W1981159481 @default.
- W2144871911 cites W1985525783 @default.
- W2144871911 cites W1987187013 @default.
- W2144871911 cites W1987383981 @default.
- W2144871911 cites W1994325599 @default.
- W2144871911 cites W1994475521 @default.
- W2144871911 cites W1995049488 @default.
- W2144871911 cites W1995312667 @default.
- W2144871911 cites W1995446793 @default.
- W2144871911 cites W1995733854 @default.
- W2144871911 cites W1996306525 @default.
- W2144871911 cites W2001196488 @default.
- W2144871911 cites W2001746733 @default.
- W2144871911 cites W2001815035 @default.
- W2144871911 cites W2004991496 @default.
- W2144871911 cites W2005882881 @default.
- W2144871911 cites W2009203772 @default.
- W2144871911 cites W2010603768 @default.
- W2144871911 cites W2013581108 @default.
- W2144871911 cites W2014821877 @default.
- W2144871911 cites W2017066766 @default.
- W2144871911 cites W2018144815 @default.
- W2144871911 cites W2019965720 @default.
- W2144871911 cites W2020714104 @default.
- W2144871911 cites W2022569090 @default.
- W2144871911 cites W2023745296 @default.
- W2144871911 cites W2024972288 @default.
- W2144871911 cites W2026721335 @default.
- W2144871911 cites W2027148204 @default.
- W2144871911 cites W2027609548 @default.
- W2144871911 cites W2031762355 @default.
- W2144871911 cites W2032832578 @default.
- W2144871911 cites W2040444511 @default.
- W2144871911 cites W2042674494 @default.
- W2144871911 cites W2045441687 @default.
- W2144871911 cites W2047314299 @default.
- W2144871911 cites W2047985534 @default.
- W2144871911 cites W2048451022 @default.
- W2144871911 cites W2049902028 @default.
- W2144871911 cites W2050162789 @default.
- W2144871911 cites W2052042341 @default.
- W2144871911 cites W2052926897 @default.
- W2144871911 cites W2057154619 @default.
- W2144871911 cites W2058314850 @default.
- W2144871911 cites W2060846115 @default.
- W2144871911 cites W2062439144 @default.
- W2144871911 cites W2063881344 @default.
- W2144871911 cites W2064700675 @default.
- W2144871911 cites W2066231779 @default.
- W2144871911 cites W2067492770 @default.
- W2144871911 cites W2069208947 @default.
- W2144871911 cites W2069982826 @default.
- W2144871911 cites W2070650982 @default.
- W2144871911 cites W2071533525 @default.
- W2144871911 cites W2072495082 @default.
- W2144871911 cites W2075221872 @default.
- W2144871911 cites W2075962899 @default.
- W2144871911 cites W2076828451 @default.
- W2144871911 cites W2078855713 @default.
- W2144871911 cites W2079476663 @default.
- W2144871911 cites W2080718709 @default.
- W2144871911 cites W2082604045 @default.
- W2144871911 cites W2082929737 @default.
- W2144871911 cites W2083842098 @default.
- W2144871911 cites W2087423786 @default.
- W2144871911 cites W2088454879 @default.
- W2144871911 cites W2089415780 @default.
- W2144871911 cites W2089521373 @default.
- W2144871911 cites W2089629668 @default.
- W2144871911 cites W2090086774 @default.
- W2144871911 cites W2093277217 @default.