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Lightcurves of stars in the Chamaeleon I association

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F25%3A00141444" target="_blank" >RIV/00216224:14310/25:00141444 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.1016/j.newast.2025.102409" target="_blank" >https://doi.org/10.1016/j.newast.2025.102409</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1016/j.newast.2025.102409" target="_blank" >10.1016/j.newast.2025.102409</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Lightcurves of stars in the Chamaeleon I association

  • Original language description

    Star-forming regions are essential for studying very young stellar objects of various masses. They still contain a significant amount of dust and gas. We present a study of light curves of stars in the field of the Chamaeleon I association. We use automatic spectral classification with MKCLASS to identify the spectral types of the stars in the field with a light curve from the NEOWISE and Gaia surveys. The light curves are analysed using the software Peranso and astropy. We also used VSX to identify the variability type. Based on astrometry, we have identified 92 stars, 73 of which are members of the association. We received light curves for 55 stars from the Gaia survey and for 69 stars from the ALLWISE/NEOWISE survey. For 28 of them, it was possible to determine the types of variables, mostly T Tauri and Orion variables. The spectral types of the members are mostly cooler M-type stars, with one being a possible chemically peculiar (CP) star. The non-members associated with light curve measurements include spectral types A-G with one CP candidate.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/GA23-07605S" target="_blank" >GA23-07605S: The fate of Galactic open clusters</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>S - Specificky vyzkum na vysokych skolach

Others

  • Publication year

    2025

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    New Astronomy

  • ISSN

    1384-1076

  • e-ISSN

    1384-1092

  • Volume of the periodical

    120

  • Issue of the periodical within the volume

    November

  • Country of publishing house

    NL - THE KINGDOM OF THE NETHERLANDS

  • Number of pages

    15

  • Pages from-to

    102409

  • UT code for WoS article

    001505069000001

  • EID of the result in the Scopus database

    2-s2.0-105005015301