Matches in SemOpenAlex for { <https://semopenalex.org/work/W4292190216> ?p ?o ?g. }
- W4292190216 endingPage "L12" @default.
- W4292190216 startingPage "L12" @default.
- W4292190216 abstract "Abstract The presence of a strong magnetic field is a feature common to a significant fraction of degenerate stars, yet little is understood about the field’s origin and evolution. New observational constraints from volume-limited surveys point to a more complex situation than a single mechanism valid for all stars. We show that in high-mass white dwarfs, which are probably the results of mergers, magnetic fields are extremely common and very strong and appear immediately in the cooling phase. These fields may have been generated by a dynamo active during the merging. Lower-mass white dwarfs, which are often the product of single-star evolution, are rarely detectably magnetic at birth, but fields appear very slowly, and very weakly, in about a quarter of them. What we may see is an internal field produced in an earlier evolutionary stage that gradually relaxes to the surface from the interior. The frequency and strength of magnetic fields continue to increase to eventually rival those of highly massive stars, particularly after the stars cool past the start of core crystallization, an effect that could be responsible for a dynamo mechanism similar to the one that is active in Earth’s interior." @default.
- W4292190216 created "2022-08-18" @default.
- W4292190216 creator A5014887556 @default.
- W4292190216 creator A5031474913 @default.
- W4292190216 date "2022-08-01" @default.
- W4292190216 modified "2023-09-30" @default.
- W4292190216 title "Multiple Channels for the Onset of Magnetism in Isolated White Dwarfs" @default.
- W4292190216 cites W1515675433 @default.
- W4292190216 cites W1626761104 @default.
- W4292190216 cites W1760900824 @default.
- W4292190216 cites W1965028497 @default.
- W4292190216 cites W1967091908 @default.
- W4292190216 cites W1967987961 @default.
- W4292190216 cites W1975583263 @default.
- W4292190216 cites W1975950228 @default.
- W4292190216 cites W1992233408 @default.
- W4292190216 cites W2000750617 @default.
- W4292190216 cites W2003687457 @default.
- W4292190216 cites W2016948475 @default.
- W4292190216 cites W2023168374 @default.
- W4292190216 cites W2025467069 @default.
- W4292190216 cites W2038518087 @default.
- W4292190216 cites W2042917575 @default.
- W4292190216 cites W2047826090 @default.
- W4292190216 cites W2057580310 @default.
- W4292190216 cites W2061767396 @default.
- W4292190216 cites W2070103975 @default.
- W4292190216 cites W2074235955 @default.
- W4292190216 cites W2077238955 @default.
- W4292190216 cites W2082954874 @default.
- W4292190216 cites W2083196057 @default.
- W4292190216 cites W2088881159 @default.
- W4292190216 cites W2090869443 @default.
- W4292190216 cites W2101439538 @default.
- W4292190216 cites W2106365190 @default.
- W4292190216 cites W2108687862 @default.
- W4292190216 cites W2113945936 @default.
- W4292190216 cites W2142722860 @default.
- W4292190216 cites W2161517877 @default.
- W4292190216 cites W2164393310 @default.
- W4292190216 cites W2170808767 @default.
- W4292190216 cites W2227238449 @default.
- W4292190216 cites W2588826510 @default.
- W4292190216 cites W2606047231 @default.
- W4292190216 cites W2799064114 @default.
- W4292190216 cites W2900082529 @default.
- W4292190216 cites W2914453771 @default.
- W4292190216 cites W2955529626 @default.
- W4292190216 cites W3030528044 @default.
- W4292190216 cites W3042167535 @default.
- W4292190216 cites W3092264406 @default.
- W4292190216 cites W3095871793 @default.
- W4292190216 cites W3098955991 @default.
- W4292190216 cites W3099109002 @default.
- W4292190216 cites W3099783027 @default.
- W4292190216 cites W3101126800 @default.
- W4292190216 cites W3101355367 @default.
- W4292190216 cites W3102813487 @default.
- W4292190216 cites W3105117504 @default.
- W4292190216 cites W3122737444 @default.
- W4292190216 cites W3124148568 @default.
- W4292190216 cites W3166651772 @default.
- W4292190216 cites W3175813211 @default.
- W4292190216 cites W4250759262 @default.
- W4292190216 cites W4280553397 @default.
- W4292190216 cites W4288083737 @default.
- W4292190216 cites W4288102915 @default.
- W4292190216 cites W4288278696 @default.
- W4292190216 cites W4289455534 @default.
- W4292190216 doi "https://doi.org/10.3847/2041-8213/ac84d3" @default.
- W4292190216 hasPublicationYear "2022" @default.
- W4292190216 type Work @default.
- W4292190216 citedByCount "13" @default.
- W4292190216 countsByYear W42921902162022 @default.
- W4292190216 countsByYear W42921902162023 @default.
- W4292190216 crossrefType "journal-article" @default.
- W4292190216 hasAuthorship W4292190216A5014887556 @default.
- W4292190216 hasAuthorship W4292190216A5031474913 @default.
- W4292190216 hasBestOaLocation W42921902161 @default.
- W4292190216 hasConcept C110472602 @default.
- W4292190216 hasConcept C115260700 @default.
- W4292190216 hasConcept C121332964 @default.
- W4292190216 hasConcept C1276947 @default.
- W4292190216 hasConcept C135757623 @default.
- W4292190216 hasConcept C150846664 @default.
- W4292190216 hasConcept C197162081 @default.
- W4292190216 hasConcept C197445014 @default.
- W4292190216 hasConcept C26873012 @default.
- W4292190216 hasConcept C44870925 @default.
- W4292190216 hasConcept C49674690 @default.
- W4292190216 hasConcept C62520636 @default.
- W4292190216 hasConceptScore W4292190216C110472602 @default.
- W4292190216 hasConceptScore W4292190216C115260700 @default.
- W4292190216 hasConceptScore W4292190216C121332964 @default.
- W4292190216 hasConceptScore W4292190216C1276947 @default.
- W4292190216 hasConceptScore W4292190216C135757623 @default.
- W4292190216 hasConceptScore W4292190216C150846664 @default.
- W4292190216 hasConceptScore W4292190216C197162081 @default.