Observing and modelling magnetic fields in white dwarfs
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F18%3A00495887" target="_blank" >RIV/67985815:_____/18:00495887 - isvavai.cz</a>
Alternative codes found
RIV/00216224:14310/18:00102570
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Observing and modelling magnetic fields in white dwarfs
Original language description
Our ongoing spectroscopic survey of high proper motion stars is a rich source of new magnetic white dwarfs. We present a few examples among cool white dwarfs showing the effect of field strength and geometry on the observed optical spectrum. Modelling of hydrogen and heavy element spectral lines reveals a range of uniform or markedly offset dipole fields in these objects.
Czech name
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
<a href="/en/project/GA15-15943S" target="_blank" >GA15-15943S: Modelling and evolution of magnetic fields in hydrogen-rich and polluted white dwarfs</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Others
Publication year
2018
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Contributions of the Astronomical Observatory Skalnaté Pleso
ISSN
1335-1842
e-ISSN
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Volume of the periodical
48
Issue of the periodical within the volume
1
Country of publishing house
SK - SLOVAKIA
Number of pages
5
Pages from-to
307-311
UT code for WoS article
000432791300055
EID of the result in the Scopus database
2-s2.0-85042661226