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Resolving binary systems down to Milli-Arcsecond precision through Stellar Intensity Interferometry with MAGIC and LST-1

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F25%3A00646029" target="_blank" >RIV/67985815:_____/25:00646029 - isvavai.cz</a>

  • Alternative codes found

    RIV/68378271:_____/25:00646029 RIV/61989592:15310/25:73635276

  • Result on the web

    <a href="https://pos.sissa.it/501/957/pdf" target="_blank" >https://pos.sissa.it/501/957/pdf</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.22323/1.501.0957" target="_blank" >10.22323/1.501.0957</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Resolving binary systems down to Milli-Arcsecond precision through Stellar Intensity Interferometry with MAGIC and LST-1

  • Original language description

    We report on recent simulations and future prospects in Stellar Intensity Interferometry (SII) using the MAGIC and LST1 telescopes to study hot, massive binary systems. Through nanosecond-scale photon correlation measurements across long baselines, we aim to resolve sub-milliarcsecond stel- lar features and constrain key binary parameters, including angular separation, radii, and brightness ratios. Simulations of the spectroscopic binary alfa Virginis (Spica) illustrate the capability of SII to resolve close binaries and validate models of stellar evolution. With the MAGIC–LST1 interfer- ometer, we also aim to identify interacting binary systems exhibiting wind collisions or Roche lobe overflow: environments that may host particle acceleration and produce very-high-energy (VHE, E > 20 GeV) gamma-ray emission. Moreover, the short-period massive binaries accessible to SII are often progenitors of compact systems such as neutron star binaries or X-ray binaries, which are themselves key targets for VHE astroparticle-physics 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

    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

    2025

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    Proceedings of Science

  • ISBN

  • ISSN

    1824-8039

  • e-ISSN

  • Number of pages

    11

  • Pages from-to

    957

  • Publisher name

    Sissa Medilab srl

  • Place of publication

    Trieste

  • Event location

    Ženeva

  • Event date

    Jul 15, 2025

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article