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Long-term observations of the classical nova X Serand the activity of post-novae

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21230%2F21%3A00350269" target="_blank" >RIV/68407700:21230/21:00350269 - isvavai.cz</a>

  • Alternative codes found

    RIV/67985815:_____/21:00552976

  • Result on the web

    <a href="https://doi.org/10.22323/1.368.0037" target="_blank" >https://doi.org/10.22323/1.368.0037</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.22323/1.368.0037" target="_blank" >10.22323/1.368.0037</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Long-term observations of the classical nova X Serand the activity of post-novae

  • Original language description

    We show a relation of the classical nova outbursts and the activity of post-novae. A variety of theoptical activities of post-novae exists. Also large changes of the type of activity in the decadesafter the classical nova outburst are observed in some of them. Although the ensemble of systemsin this analysis is incomplete, the similarities in the decaying branches of the outbursts in somepost-novae are the features favoring the dwarf nova outbursts. The features consistent with thedwarf nova outbursts appear mainly in the later phases (years, decades) of the gradual decay ofthe mean luminosity of some post-novae. This suggests that they contain the accretion diskswhich were able to switch from the hot (ionized) state to the thermal-viscous instability (TVI)regime. Such a TVI of the disk can appear in some post-novae even during the first century afterthe classical nova outburst (often sooner after the classical nova outburst in cataclysmic variableswith longer orbital periods). Activity of the mass-donating star in the brightness variations ofsome post-novae can be caused by the appearance and changes of the position of the active regionson the donor.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/GA17-05840S" target="_blank" >GA17-05840S: Multicriteria Optimization of Shift-Variant Imaging System Models</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2021

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    5th Golden Age of Cataclysmic Variables and Related Objects

  • ISBN

  • ISSN

    1824-8039

  • e-ISSN

    1824-8039

  • Number of pages

    11

  • Pages from-to

  • Publisher name

    Proceedings of Science

  • Place of publication

    Trieste

  • Event location

    Palermo

  • Event date

    Sep 2, 2019

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article