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Related papers: The extended Main-Sequence Turnoff of the Milky Wa…

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We present photometric analysis of twelve Galactic open clusters and show that the same multiple-population phenomenon observed in Magellanic Clouds (MCs) is present in nearby open clusters. Nearly all the clusters younger than $\sim$2.5…

Solar and Stellar Astrophysics · Physics 2018-12-26 G. Cordoni , A. P. Milone , A. F. Marino , M. Di Criscienzo , F. D'Antona , A. Dotter , E. P. Lagioia , M. Tailo

We report the serendipitous young Large Magellanic Cloud cluster, NGC 1971, exhibits an extended main-sequence turnoff (eMSTO) possibly originated by mostly a real age spread. We used CT1 Washington photometry to produce a colour-magnitude…

Astrophysics of Galaxies · Physics 2017-07-26 Andrés E. Piatti , Andrew Cole

Recent Gaia photometry of the open cluster M37 have disclosed the existence of an extended main-sequence turn off -- like in Magellanic clusters younger than about 2 Gyr -- and a main sequence that is broadened in colour beyond what is…

Solar and Stellar Astrophysics · Physics 2022-09-21 M. Griggio , M. Salaris , S. Cassisi , A. Pietrinferni , L. R. Bedin

We present results on the age and metallicity estimates of the poorly studied LMC cluster SL 529, from CCD SDSS gr photometry obtained at the Gemini South telescope with the GMOS attached. The cluster MSTO region possesses an extended…

Astrophysics of Galaxies · Physics 2015-06-12 Andrés E. Piatti

The extended main sequence (eMS) and extended main sequence turnoff (eMSTO) phenomena have been observed in some young and intermediate-age star clusters in the Milky Way and in the Magellanic Clouds. In this study, we conduct a survey of…

Astrophysics of Galaxies · Physics 2026-04-07 Khushboo K Rao , Wen-Ping Chen

We report astrophysical properties of 12 Milky Way open clusters located beyond the circle around the Sun where the number of catalogued open clusters is thought to be statistically complete. By using deep optical photometry, we estimated…

Astrophysics of Galaxies · Physics 2019-07-31 Andrés E. Piatti , Mateus S. Angelo , Wilton S. Dias

The origin of extended main-sequence turn-offs (eMSTO) in star clusters younger than 2 Gyr still challenges our current understanding of stellar evolution. Exploiting data from Gaia Data Release 3 (DR3), we investigate eMSTOs in a large…

We present Hubble Space Telescope photometry of NGC1850, a ~100 Myr, ~10^5 Msun cluster in the Large Magellanic Cloud. The colour magnitude diagram clearly shows the presence of an extended main sequence turnoff (eMSTO). The use of…

We investigate the morphology of the colour-magnitude diagram (CMD) of the open cluster NGC 2509 in comparison with other Galactic open clusters of similar age using Gaia photometry. At $\sim900$ Myr Galactic open clusters in our sample all…

Solar and Stellar Astrophysics · Physics 2020-01-08 M. de Juan Ovelar , S. Gossage , S. Kamann , N. Bastian , C. Usher , I. Cabrera-Ziri , C. Conroy , C. Lardo

We use the Wide Field Camera 3 onboard the Hubble Space Telescope to obtain deep, high-resolution photometry of the young (~ 100 Myr) star cluster NGC1850 in the Large Magellanic Cloud. We analyze the cluster colour-magnitude diagram (CMD)…

Solar and Stellar Astrophysics · Physics 2017-01-18 Matteo Correnti , Paul Goudfrooij , Andrea Bellini , Jason S. Kalirai , Thomas H. Puzia

The color-magnitude diagrams (CMDs) of intermediate-age star clusters (less than ~ 2 Gyr) are much more complex than those predicted by coeval, nonrotating stellar evolution models. Their observed extended main sequence turnoffs (eMSTOs)…

Solar and Stellar Astrophysics · Physics 2022-08-03 Mikhail Lipatov , Timothy D. Brandt , Seth Gossage

Main sequence turn-off (MSTO) stars are good tracers of Galactic populations since their ages can be reliably estimated from atmospheric parameters. Based on the GALAH survey, we use the Yale Rotation Evolution Code to determine ages of…

Solar and Stellar Astrophysics · Physics 2022-04-27 Xunzhou Chen , Zhishuai Ge , Yuqin Chen , Shaolan Bi , Jie Yu , Wuming Yang , Jason W. Ferguson , Yaqian Wu , Yaguang Li

We present color-magnitude diagram analysis of deep Hubble Space Telescope imaging of a mass-limited sample of 18 intermediate-age (1 - 2 Gyr old) star clusters in the Magellanic Clouds, including 8 clusters for which new data was obtained.…

In this study, we have used the {\it Gaia} Third Data Release (Gaia DR3) to investigate an intermediate-age open cluster Collinder 74. Taking into account the stars with membership probabilities over 0.5 and inside the limiting radius of…

Astrophysics of Galaxies · Physics 2023-10-23 T. Yontan , R. Canbay

We present an analysis of the relatively low mass ($\sim2400$~M$_{\odot}$), $\sim800$~Myr, Galactic open cluster, NGC~2818, using Gaia DR2 results combined with VLT/FLAMES spectroscopy. Using Gaia DR2 proper motions and parallax…

Solar and Stellar Astrophysics · Physics 2018-08-08 N. Bastian , S. Kamann , I. Cabrera-Ziri , C. Georgy , S. Ekström , C. Charbonnel , M. de Juan Ovelar , C. Usher

Recent studies have shown that the extended main-sequence turn off (eMSTO) is a common feature of intermediate-age star clusters in the Magellanic Clouds (MCs). The most simple explanation is that these stellar systems harbor multiple…

Solar and Stellar Astrophysics · Physics 2015-05-27 A. P. Milone , L. R. Bedin , G. Piotto , A. F. Marino , S. Cassisi , A. Bellini , H. Jerjen , A. Pietrinferni , A. Aparicio , R. M. Rich

We present the analysis of an eccentric, partially eclipsing long-period ($P=19.23$ d) binary system KIC 9777062 that contains main sequence stars near the turnoff of the intermediate age open cluster NGC 6811. The primary is a metal-lined…

Recent studies indicate that some Galactic open clusters (OCs) exhibit extended main-sequence turnoff (eMSTO) in their colour-magnitude diagrams (CMDs). However, the number of Galactic OCs with eMSTO structures detected so far is limited,…

Solar and Stellar Astrophysics · Physics 2024-04-11 Yangyang Deng , Zhongmu Li

The extended main-sequence turn-off (eMSTO) is a well-known feature observed in young and intermediate-age star clusters, characterized by a significant broadening of the main-sequence turn-off region. Although prolonged star formation and…

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