Please use this identifier to cite or link to this item:https://hdl.handle.net/20.500.12259/103280
 Type of publication: Straipsnis Clarivate Analytics Web of Science ar/ir Scopus / Article in Clarivate Analytics Web of Science or / and Scopus (S1) Field of Science: Astronomija / Astronomy (N008) Author(s): Straižys, Vytautas;Boyle, R. P;Raudeliūnas, S;Zdanavičius, J;Janusz, R;Macijauskas, M;Lazauskaitė, Romualda;Černis, K;Zdanavičius, K;Maskoliūnas, M;Čepas, V;Kazlauskas, A Title: Open cluster IC 1369 and its vicinity: multicolor photometry and Gaia DR2 astrometry Is part of: Astronomical journal Bristol : IOP Publishing Ltd, 2020, vol. 159, No. 3, article No. 95 Extent: p. 1-9 Date: 2020 Keywords: Open star clusters;Stellar classification;Hertzsprung Russell diagram;Interstellar dust extinction Abstract: The open cluster IC 1369, located in Cygnus close to the galactic equator at the 89fdg6 longitude, and its vicinity are investigated by applying two-dimensional photometric classification of stars down to V = 19 mag measured in the Vilnius seven-color photometric system. Employing the Gaia DR2 coordinates, parallaxes, and proper motions, 143 cluster members are found having cluster membership probabilities ≥0.75. The hottest stars of the evolved main sequence are of spectral class B9. Distances to the cluster, determined by two methods based on the Gaia parallaxes, are 3280 and 3370 pc with an uncertainty of 400–500 pc. Employing the physical HR diagram with the coordinates $\mathrm{log}L/{L}_{\odot }$ versus $\mathrm{log}{T}_{\mathrm{eff}}$ and the Padova isochrones, the cluster age is found to be between 300 and 350 Myr. Among the cluster members we identified six red giants of spectral classes G5–G8 and luminosities II–III, 17 Am stars, one Ap star, and one B5 blue straggler. The extinction shows a steep rise up to ~2.0 mag at 300–700 pc, caused by the extensions of the dust cloud LDN 970 and the Great Cygnus Rift, and up to ~2.5 mag at the edge of the Perseus arm at 3.0 kpc. The extinction is almost constant between 0.9 and 2.5 kpc from the Sun. The average extinction of the cluster members is 2.54 mag. A systematic error of color excesses found in the Argonaut calculator results is discussed Internet: https://iopscience.iop.org/article/10.3847/1538-3881/ab67b5/pdfhttps://doi.org/10.3847/1538-3881/ab67b5 Affiliation(s): Mokytojų rengimo institutasVilniaus universiteto astronomijos observatorijaVytauto Didžiojo universitetas Appears in Collections: Universiteto mokslo publikacijos / University Research Publications

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