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A New Look into the Spectral and Light Variations of varepsilon Aur

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F13%3A00399946" target="_blank" >RIV/67985815:_____/13:00399946 - isvavai.cz</a>

  • Result on the web

  • DOI - Digital Object Identifier

Alternative languages

  • Result language

    angličtina

  • Original language name

    A New Look into the Spectral and Light Variations of varepsilon Aur

  • Original language description

    Investigating long series of spectral and photometric observations, we found that the orbital elements of /varepsilon Aur are subject to much larger uncertainties than usually believed. The H? emission is found to move basically with the F primary but its exact location should still be investigated. We also find strong additional absorption and large reddening of the object near the third contact during the eclipse. Episodic atmospheric mass transfer from the F primary towards its companion is tentatively suggested.

  • 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

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2013

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Central European Astrophysical Bulletin

  • ISSN

    1845-8319

  • e-ISSN

  • Volume of the periodical

    37

  • Issue of the periodical within the volume

    1

  • Country of publishing house

    HR - CROATIA

  • Number of pages

    10

  • Pages from-to

    99-108

  • UT code for WoS article

  • EID of the result in the Scopus database