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Astrophysics of “Extreme Solar-Like Stars

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F16%3A00470694" target="_blank" >RIV/67985815:_____/16:00470694 - isvavai.cz</a>

  • Alternative codes found

    RIV/68407700:21230/16:00307321

  • Result on the web

  • DOI - Digital Object Identifier

Alternative languages

  • Result language

    angličtina

  • Original language name

    Astrophysics of “Extreme Solar-Like Stars

  • Original language description

    Only a few red dwarf flaring stars in the solar neighbourhood have undergone exceptional events called superflares. They have been detected with high-energy satellites (Swift) and have been proven to be powerful events (both in intensity and energy) and potentially hazardous for any extra terrestial life. The physics of these events can be understood as an extrapolation of the (much) weaker activity already occurring in the most powerful solar flares occurring in the Sun. Nevertheless, the origin (why?) of these superflares occur isncurrently unknown. A recent study presents the optical and X-ray long-term evolution of the emission by the super-flare from the red-dwarf star DG CVn undertaken in 2 014. In that paper we comment on the context of these observations and on the properties that can be derived through the analysis of them.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2016

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Revista Mexicana de Astronomia y Astrofisica Serie de Conferencias

  • ISSN

    1405-2059

  • e-ISSN

  • Volume of the periodical

    48

  • Issue of the periodical within the volume

    2

  • Country of publishing house

    MX - MEXICO

  • Number of pages

    5

  • Pages from-to

    59-63

  • UT code for WoS article

  • EID of the result in the Scopus database