A search for kilogauss magnetic fields in white dwarfs and hot subdwarf stars

Simple item page
dc.creatorValyavin, G.
dc.creatorBagnulo, S.
dc.creatorFabrika, S.
dc.creatorReisenegger, A.
dc.creatorWade, G. A.
dc.creatorHan, Inwoo
dc.creatorMonin, D.
dc.date2006-05-16
dc.date.accessioned2026-07-07T10:39:01Z
dc.date.available2026-07-07T10:39:01Z
dc.descriptionWe present new results of a survey for weak magnetic fields among DA white dwarfs with inclusion of some brighter hot subdwarf stars. We have detected variable circular polarization in the Halpha line of the hot subdwarf star Feige 34 (SP: sdO). From these data, we estimate that the longitudinal magnetic field of this star varies from -1.1 +/- 3.2 kG to +9.6 +/- 2.6 kG, with a mean of about +5 kG and a period longer than 2 h. In this study, we also confirm the magnetic nature of white dwarf WD1105-048 and present upper limits of kilogauss longitudinal magnetic fields of 5 brightest DA white dwarfs. Our data support recent finding that 25% of white dwarfs have kilogauss magnetic fields. This frequency also confirms results of early estimates obtained using the magnetic field function of white dwarfs.
dc.descriptionaccepted for publication in the Astrphysical Journal
dc.identifierhttps://arxiv.org/abs/astro-ph/0605401
dc.identifierhttp://arxiv.org/abs/astro-ph/0605401
dc.identifierAstrophys.J.648:559-564,2006
dc.identifierdoi:10.1086/505781
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/180885
dc.subjectAstrophysics
dc.titleA search for kilogauss magnetic fields in white dwarfs and hot subdwarf stars
dc.typetext

Files

Collections

arXiv