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17th European White Dwarf Workshop: New insights on the origin of magnetic fields in white dwarfs and neutron stars
Wickramasinghe, Dayal (2010)
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mla
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Wickramasinghe D. "17th European White Dwarf Workshop: New insights on the origin of magnetic fields in white dwarfs and neutron stars.", timms video, Universität Tübingen (2010): https://timms.uni-tuebingen.de:443/tp/UT_20100817_001_eurowd_0001. Accessed 30 Nov 2020.
apa
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Wickramasinghe, D. (2010). 17th European White Dwarf Workshop: New insights on the origin of magnetic fields in white dwarfs and neutron stars. timms video: Universität Tübingen. Retrieved November 30, 2020 from the World Wide Web https://timms.uni-tuebingen.de:443/tp/UT_20100817_001_eurowd_0001
harvard
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Wickramasinghe, D. (2010). 17th European White Dwarf Workshop: New insights on the origin of magnetic fields in white dwarfs and neutron stars [Online video]. 17 August. Available at: https://timms.uni-tuebingen.de:443/tp/UT_20100817_001_eurowd_0001 (Accessed: 30 November 2020).
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title: 17th European White Dwarf Workshop: New insights on the origin of magnetic fields in white dwarfs and neutron stars
alt. title: 17th European White Dwarf Workshop - White dwarf structure and evolution
creator: Wickramasinghe, Dayal (author)
subjects: Astronomie, Physik, Astrophysik, Workshop, White Dwarf, magnetic fields, neutron stars, Dayal Wickramasinghe
description: 17th European White Dwarf Workshop, 16. bis 20. August 2010
abstract: New insights on the origin of magnetic fields in white dwarfs and neutron stars (Dayal Wickramasinghe and Lilia Ferrario) (Mathematical Sciences Institute, The Australian National University, ACT 0200, Australia) Main sequence, white dwarf and neutron stars are observed to exhibit a wide range of magnetic fluxes with a maximum that appears to be remarkably insensitive to the type of star. We discuss these observations in the context of the fossil and dynamo hypotheses for the origin of magnetic fields in stars, and discuss the role played by mergers in the amplification of magnetic fields. We propose that the magnetic fields of the high field and low field magnetic white dwarfs are likely to have different origins and discuss possible scenarios that may explain current observations.
publisher: ZDV Universität Tübingen
contributor: ZDV Universität Tübingen (producer)
creation date: 2010-08-17
dc type: image
localtype: video
identifier: UT_20100817_001_eurowd_0001
language: eng
rights: Url: https://timmsstatic.uni-tuebingen.de/jtimms/TimmsDisclaimer.html?637423594428908991