Comprehensive Analysis of the Open Cluster Collinder 74

Year 2023, , 65 - 73, 21.12.2023

Talar Yontan , Remziye Canbay

https://doi.org/10.26650/PAR.2023.00008

Abstract

In this study, we have used the Gaia Third Data Release (Gaia DR3) to investigate an intermediate-age open cluster Collinder 74. We have identified 102 probable cluster members by considering stars with a membership probability exceeding 0.5 and located within the designated confinement radius. The mean proper-motion components of Collinder 74 are estimated as (𝜇𝛼 cos 𝛿, 𝜇𝛿) = (0.960 ± 0.005, −1.526 ± 0.004) mas yr−1 . We detected previously confirmed four blue straggler stars which show flat radial distribution. Colour excess, distance, and age of the cluster were estimated simultaneously by fitting PARSEC isochrones to the observational data on Gaia based colour magnitude diagram. These values were derived as 𝐸(𝐺BP − 𝐺RP) = 0.425 ± 0.046 mag, 𝑑 = 2831 ± 118 pc and 𝑡 = 1800 ± 200 Myr, respectively. The mass function slope was estimated as Γ = 1.34 ± 0.21 within the mass range 0.65 ≤ 𝑀/𝑀⊙ ≤ 1.58 which is well matched with that of Salpeter. Stellar mass distribution indicated that the massive and most likely stars are concentrated around the cluster center. The total mass of the cluster was found to be 365 𝑀/𝑀⊙ for the stars with probabilities 𝑃 > 0. Galactic orbit integration shows that the Collinder 74 follows a boxy pattern outside the solar circle and is a member of the thin-disc component of the Galaxy.

Keywords

Galaxy, open clusters and associations, individual, Collinder 74; stars, Hertzsprung Russell (HR) diagram, Stellar kinematics

References

• Ann H. B., Lee M. G., Chun M. Y., Kim S. L., Jeon Y. B., Park B. G., 1999, Journal of Korean Astronomical Society, 32, 7 google scholar
• Bilir S., Karaali S., Ak S., Yaz E., Hamzaoğlu E., 2006a, New Astron., 12, 234 google scholar Bilir S., Karaali S., Gilmore G., 2006b, MNRAS, 366, 1295 google scholar
• Bilir S., Cabrera-Lavers A., Karaali S., Ak S., Yaz E., Lopez- google scholar
• Corredoira M., 2008, Publ. Astron. Soc. Australia, 25, 69 google scholar
• Bisht D., Yadav R. K. S., Ganesh S., Durgapal A. K., Rangwal G., Fynbo J. P. U., 2019, MNRAS, 482, 1471 google scholar
• Bisht D., Zhu Q., Yadav R. K. S., Durgapal A., Rangwal G., 2020, MNRAS, 494, 607 google scholar
• Bovy J., 2015, ApJS, 216, 29 google scholar
• Bovy J., Tremaine S., 2012, ApJ, 756, 89 google scholar
• Bressan A., Marigo P., Girardi L., Salasnich B., Dal Cero C., Rubele google scholar
• S., Nanni A., 2012, MNRAS, 427, 127 google scholar
• Cantat-Gaudin T., et al., 2018, A&A, 618, A93 google scholar
• Cantat-Gaudin T., et al., 2020, A&A, 640, A1 google scholar
• Carraro G., Costa E., 2007, A&A, 464, 573 google scholar
• Carraro G., Sales Silva J. V., Moni Bidin C., Vazquez R. A., 2017, AJ, 153, 99 google scholar
• Coşkunoglu B., et al., 2011, MNRAS, 412, 1237 google scholar
• Dias W. S., Assafin M., Florio V., Alessi B. S., Libero V., 2006, A&A, 446, 949 google scholar
• Dias W. S., Monteiro H., Caetano T. C., Lepine J. R. D., Assafin M., Oliveira A. F., 2014, A&A, 564, A79 google scholar
• Dias W. S., Monteiro H., Assafin M., 2018, MNRAS, 478, 5184 google scholar
• Dias W. S., Monteir H., Moitinho A., Lepine J. R. D., Carraro G., google scholar
• Paunzen E., Alessi B., Villela L., 2021, MNRAS, 504, 356 google scholar
• Ferraro F. R., et al., 2012, Nature, 492, 393 google scholar
• Gaia Collaboration et al., 2016, A&A, 595, A1 google scholar
• Gaia Collaboration et al., 2018, A&A, 616, A1 google scholar
• Gaia Collaboration et al., 2023, A&A, 674, A1 google scholar
• Hasegawa T., Sakamoto T., Malasan H. L., 2008, PASJ, 60, 1267 google scholar
• Hills J. G., Day C. A., 1976, Astrophys. Lett., 17, 87 google scholar
• Hunt E. L., Reffert S., 2023, A&A, 673, A114 google scholar
• Jadhav V. V., Subramaniam A., 2021, MNRAS, 507, 1699 google scholar
• Juric M., et al., 2008, ApJ, 673, 864 google scholar
• Kharchenko N. V., Piskunov A. E., Schilbach E., Röser S., Scholz R. D., 2013, A&A, 558, A53 google scholar
• Kim S. C., Kyeong J., Park H. S., Han I., Lee J. H., Moon D.-S., Lee Y., Kim S., 2017, Journal of Korean Astronomical Society, 50, 79 google scholar
• King I., 1962, AJ, 67, 471 google scholar
• Krone-Martins A., Moitinho A., 2014, A&A, 561, A57 google scholar
• Lada C. J., Lada E. A., 2003, ARA&A, 41, 57 google scholar
• Lata S., Pandey A. K., Sagar R., Mohan V., 2002, A&A, 388, 158 google scholar
• Leggett S. K., 1992, ApJS, 82, 351 google scholar
• Liu L., Pang X., 2019, ApJS, 245, 32 google scholar
• Loktin A. V., Popova M. E., 2017, Astrophysical Bulletin, 72, 257 google scholar
• Marsakov V. A., Gozha M. L., Koval’ V. V., Shpigel’ L. V., 2016, Astronomy Reports, 60, 43 google scholar
• Miyamoto M., Nagai R., 1975, PASJ, 27, 533 google scholar
• Navarro J. F., Frenk C. S., White S. D. M., 1996, ApJ, 462, 563 google scholar
• Rain M. J., Ahumada J. A., Carraro G., 2021, A&A, 650, A67 google scholar
• Salpeter E. E., 1955, ApJ, 121, 161 google scholar
• Sandage A. R., 1953, AJ, 58, 61 google scholar
• Sariya D. P., et al., 2021, AJ, 161, 101 google scholar
• Soubiran C., et al., 2018, A&A, 619, A155 google scholar
• Sun M., Jiang B., Yuan H., Li J., 2021, ApJS, 254, 38 google scholar
• Taşdemir S., Yontan T., 2023, Physics and Astronomy Reports, 1, 1 google scholar
• Tadross A. L., 2001, New Astron., 6, 293 google scholar
• Tarricq Y., et al., 2021, A&A, 647, A19 google scholar
• Zacharias N., Finch C. T., Girard T. M., Henden A., Bartlett J. L., Monet D. G., Zacharias M. I., 2013, AJ, 145, 44 google scholar
• Zhong J., Chen L., Wu D., Li L., Bai L., Hou J., 2020, A&A, 640, A127 google scholar
• Zinn R., Dahn C. C., 1976, AJ, 81, 527 google scholar