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
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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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