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Unraveling the variability of σ Ori E

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F14%3A00455509" target="_blank" >RIV/67985815:_____/14:00455509 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1017/S1743921314007066" target="_blank" >http://dx.doi.org/10.1017/S1743921314007066</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1017/S1743921314007066" target="_blank" >10.1017/S1743921314007066</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Unraveling the variability of σ Ori E

  • Original language description

    Sigma Ori E (HD 37479) is the prototypical helium-strong star shown to harbor a strong magnetic field, as well as a magnetosphere consisting of two clouds of plasma. The observed optical (ubvy) light curve of σ Ori E is dominated by eclipse features due to circumstellar material, however, there remain additional features unexplained by the Rigidly Rotating Magnetosphere (RRM) model of Townsend & Owocki (2005). Using the technique of magnetic Doppler imaging (MDI), spectropolarimetric observations of σ Ori E are used to produce maps of both the magnetic field topology and various elemental abundance distributions. We also present an analysis utilizing these computed MDI maps in conjunction with non-local thermodynamical equilibrium TLUSTY models to study the optical brightness variability of this star arising from surface inhomogeneities. It has been suggested that this physical phenomena may be responsible for the light curve inconsistencies between the model and observations.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2014

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Article name in the collection

    New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry

  • ISBN

    9781107078581

  • ISSN

    1743-9213

  • e-ISSN

  • Number of pages

    5

  • Pages from-to

    348-352

  • Publisher name

    Cambridge University Press

  • Place of publication

    Cambridge

  • Event location

    Geneva

  • Event date

    Jun 23, 2014

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article

    000453211700088