@Article{SchreiberBellGansPars:2021:ReMaPo,
author = "Schreiber, Matthias R. and Belloni, Diogo Teixeira and Gansicke,
Boris T. and Parsons, Steven G.",
affiliation = "{Universidad Tecnica Federico Santa Mar{\'{\i}}a} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {University of
Warwick} and {University of Sheffield}",
title = "Magnetic dynamos in white dwarfs - II. Relating magnetism and
pollution",
journal = "Monthly Notices of the Royal Astronomical Society",
year = "2021",
volume = "506",
number = "1",
pages = "L29--L34",
month = "Sept.",
keywords = "magnetic fields, planetary systems, white dwarfs.",
abstract = "We investigate whether the recently suggested rotation and
crystallization driven dynamo can explain the apparent increase of
magnetism in old metal polluted white dwarfs. We find that the
effective temperature distribution of polluted magnetic white
dwarfs is in agreement with most/all of them having a
crystallizing core, and increased rotational velocities are
expected due to accretion of planetary material that is evidenced
by the metal absorption lines. We conclude that a rotation and
crystallization driven dynamo offers not only an explanation for
the different occurrence rates of strongly magnetic white dwarfs
in close binaries but also for the high incidence of weaker
magnetic fields in old metal polluted white dwarfs.",
doi = "10.1093/mnrasl/slab069",
url = "http://dx.doi.org/10.1093/mnrasl/slab069",
issn = "0035-8711 and 1365-2966",
language = "en",
targetfile = "slab069.pdf",
urlaccessdate = "31 maio 2024"
}