Chemically peculiar stars as members of open clusters

J 2025

Chemically peculiar stars as members of open clusters

FALTOVÁ, Nikola; Daniel JADLOVSKÝ; L. KUESS; Matúš LABAJ; Marko MESARČ et. al.

Základní údaje

Originální název

Chemically peculiar stars as members of open clusters

Autoři

Vydání

Monthly Notices of the Royal Astronomical Society, Oxford University Press, 2025, 0035-8711

Další údaje

Jazyk

angličtina

Typ výsledku

Článek v odborném periodiku

Obor

10308 Astronomy

Stát vydavatele

Velká Británie a Severní Irsko

Utajení

není předmětem státního či obchodního tajemství

Odkazy

URL

Impakt faktor

Impact factor: 4.800 v roce 2024

Organizační jednotka

Přírodovědecká fakulta

DOI

https://doi.org/10.1093/mnras/stae2563

UT WoS

001374757200001

Klíčová slova anglicky

astronomical data bases; catalogues; stars: chemically peculiar; open clusters and associations: general

Štítky

rivok

Příznaky

Mezinárodní význam, Recenzováno

Změněno: 10. 4. 2025 12:33, Tahereh Ramezani

Anotace

V originále

The chemically peculiar (CP) stars of the upper main sequence are excellent astrophysical laboratories to test the diffusion, mass-loss, rotational mixing, and pulsation in the (non-)presence of a stable local magnetic field. These processes are time-dependent. The age estimation of Galactic field stars suffers from several limitations. Therefore, studying members of star clusters overcomes these difficulties. We matched the most recently published catalogues of star clusters and CP stars. For the matching, we used the newest Gaia Data Release. We also used the delta a photometry tool to further distinguish between the CP subgroups. We found 595 CP stars in 408 star clusters of all ages. Furthermore, we report on misclassified metallic line stars (Am or CP1) and objects with no CP classification. The distribution of magnetic and non-magnetic CP stars on the main sequence seems different. We do not detect very young and very old CP stars showing rotationally induced variability. CP members of star clusters help to study all relevant processes responsible for this phenomenon in more detail. Still, a larger sample is desired to put tighter constraints on models.

Návaznosti

GA23-07605S, projekt VaV

Název: Osud galaktických otevřených hvězdokup

Investor: Grantová agentura ČR, Osud galaktických otevřených hvězdokup

Citovat

FALTOVÁ, Nikola; Daniel JADLOVSKÝ; L. KUESS; Matúš LABAJ; Marko MESARČ; Prapti MONDAL; Kateřina NEUMANNOVÁ; Ernst PAUNZEN; Michal PRIŠEGEN; Tahereh RAMEZANI; Johana SUPÍKOVÁ; Kateřina SVAČINKOVÁ; Gabriel SZÁSZ; Michaela VÍTKOVÁ a Caiyun XIA. Chemically peculiar stars as members of open clusters. Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2025, roč. 536, č. 1, s. 72-78. ISSN 0035-8711. Dostupné z: https://doi.org/10.1093/mnras/stae2563.

@article{2481660,
   author = {Faltová, Nikola and Jadlovský, Daniel and Kuess, L. and Labaj, Matúš and Mesarč, Marko and Mondal, Prapti and Neumannová, Kateřina and Paunzen, Ernst and Prišegen, Michal and Ramezani, Tahereh and Supíková, Johana and Svačinková, Kateřina and Szász, Gabriel and Vítková, Michaela and Xia, Caiyun},
   article_number = {1},
   doi = {https://doi.org/10.1093/mnras/stae2563},
   keywords = {astronomical data bases; catalogues; stars: chemically peculiar; open clusters and associations: general},
   language = {eng},
   issn = {0035-8711},
   journal = {Monthly Notices of the Royal Astronomical Society},
   title = {Chemically peculiar stars as members of open clusters},
   url = {https://doi.org/10.1093/mnras/stae2563},
   volume = {536},
   year = {2025}
}

TY  - JOUR
ID  - 2481660
AU  - Faltová, Nikola - Jadlovský, Daniel - Kuess, L. - Labaj, Matúš - Mesarč, Marko - Mondal, Prapti - Neumannová, Kateřina - Paunzen, Ernst - Prišegen, Michal - Ramezani, Tahereh - Supíková, Johana - Svačinková, Kateřina - Szász, Gabriel - Vítková, Michaela - Xia, Caiyun
PY  - 2025
TI  - Chemically peculiar stars as members of open clusters
JF  - Monthly Notices of the Royal Astronomical Society
VL  - 536
IS  - 1
SP  - 72-78
EP  - 72-78
PB  - Oxford University Press
SN  - 00358711
KW  - astronomical data bases
KW  - catalogues
KW  - stars: chemically peculiar
KW  - open clusters and associations: general
UR  - https://doi.org/10.1093/mnras/stae2563
N2  - The chemically peculiar (CP) stars of the upper main sequence are excellent astrophysical laboratories to test the diffusion, mass-loss, rotational mixing, and pulsation in the (non-)presence of a stable local magnetic field. These processes are time-dependent. The age estimation of Galactic field stars suffers from several limitations. Therefore, studying members of star clusters overcomes these difficulties. We matched the most recently published catalogues of star clusters and CP stars. For the matching, we used the newest Gaia Data Release. We also used the delta a photometry tool to further distinguish between the CP subgroups. We found 595 CP stars in 408 star clusters of all ages. Furthermore, we report on misclassified metallic line stars (Am or CP1) and objects with no CP classification. The distribution of magnetic and non-magnetic CP stars on the main sequence seems different. We do not detect very young and very old CP stars showing rotationally induced variability. CP members of star clusters help to study all relevant processes responsible for this phenomenon in more detail. Still, a larger sample is desired to put tighter constraints on models.
ER  -

FALTOVÁ, Nikola; Daniel JADLOVSKÝ; L. KUESS; Matúš LABAJ; Marko MESARČ; Prapti MONDAL; Kateřina NEUMANNOVÁ; Ernst PAUNZEN; Michal PRIŠEGEN; Tahereh RAMEZANI; Johana SUPÍKOVÁ; Kateřina SVAČINKOVÁ; Gabriel SZÁSZ; Michaela VÍTKOVÁ a Caiyun XIA. Chemically peculiar stars as members of open clusters. \textit{Monthly Notices of the Royal Astronomical Society}. Oxford University Press, 2025, roč.~536, č.~1, s.~72-78. ISSN~0035-8711. Dostupné z: https://doi.org/10.1093/mnras/stae2563.

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