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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…

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…

星系天体物理 · 物理学 2026-04-07 Khushboo K Rao , Wen-Ping Chen

Extended main sequence turn-off (eMSTO) regions are a common feature in color-magnitude diagrams of young and intermediate-age star clusters in the Magellanic Clouds. The nature of eMSTOs remains debated in the literature. The currently…

星系天体物理 · 物理学 2017-08-28 Paul Goudfrooij , Leo Girardi , Matteo Correnti

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…

太阳与恒星天体物理 · 物理学 2018-08-08 N. Bastian , S. Kamann , I. Cabrera-Ziri , C. Georgy , S. Ekström , C. Charbonnel , M. de Juan Ovelar , C. Usher

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)…

太阳与恒星天体物理 · 物理学 2022-08-03 Mikhail Lipatov , Timothy D. Brandt , Seth Gossage

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.…

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…

We present an imaging analysis of four low mass stellar clusters (< 5000 Mo) in the outer regions of the LMC in order to shed light on the extended main sequence turn-off (eMSTO) phenomenon observed in high mass clusters. The four clusters…

星系天体物理 · 物理学 2016-05-11 Andrés E. Piatti , Nate Bastian

The origin of extended main sequence turnoffs (eMSTOs) in intermediate-age (1-3 Gyr) clusters is one of the most intriguing questions in current star cluster research. Unlike the split main sequences found in some globular clusters. which…

太阳与恒星天体物理 · 物理学 2019-05-15 Weijia Sun , Richard de Grijs , Licai Deng , Michael D. Albrow

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…

太阳与恒星天体物理 · 物理学 2018-12-26 G. Cordoni , A. P. Milone , A. F. Marino , M. Di Criscienzo , F. D'Antona , A. Dotter , E. P. Lagioia , M. Tailo

Stellar rotation, age spread and binary stars are thought to be three most possible causes of the peculiar color-magnitude diagrams (CMDs) of some star clusters, which exhibit extended main-sequence turn-offs (eMSTOs). It is far from…

太阳与恒星天体物理 · 物理学 2016-07-20 Zhongmu Li , Caiyan Mao , Liyun Zhang , Xi Zhang , Li Chen

Extended main sequences (eMSs) and extended main-sequence turnoffs (eMSTOs) are fascinating phenomena that are routinely observed in star clusters. These phenomena strongly challenge the current canonical "simple stellar population" picture…

太阳与恒星天体物理 · 物理学 2024-01-17 Chengyuan Li , Antonino P. Milone , Weijia Sun , Richard de Grijs

We combine a number of recent studies of the extended main sequence turn-off (eMSTO) phenomenon in intermediate age stellar ($1-2$ Gyr) clusters in the Large Magellanic Cloud (LMC) in order to investigate its origin. By employing the…

星系天体物理 · 物理学 2016-08-31 Andrés E. Piatti , Nate Bastian

The extended main sequence turn offs (eMSTOs) of several young to intermediate age clusters are examined in the Magellanic Clouds and the Milky Way. We explore the effects of extended star formation (eSF) and a range of stellar rotation…

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…

The extended main-sequence turn-offs (eMSTOs) and extended red clumps (eRCs) observed in intermediate-age star clusters challenge the traditional understanding of clusters as simple stellar populations. Recently, eMSTOs have been…

Star clusters have long been considered to comprise a simple stellar population, but this paradigm is being challenged, since apart from multiple populations in Galactic globular clusters^{1,2}, a number of intermediate-age star clusters…

太阳与恒星天体物理 · 物理学 2020-12-09 Beomdu Lim , Gregor Rauw , Yael Naze , Hwankyung Sung , Narae Hwang , Byeong-Gon Park

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…

太阳与恒星天体物理 · 物理学 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 the extended Main Sequence Turn-Off (eMSTO) in the open cluster NGC\,6067. We derive the projected rotational velocity, \textit{v}sin\textit{i}, of the stars belonging to the eMSTO region of the main sequence (MS)…

太阳与恒星天体物理 · 物理学 2025-07-22 Jayanand Maurya , Yu Zhang , Sebastian Kamann , Hubiao Niu , Yves Frémat , Kaixiang Lang , Y. C. Joshi , M. R. Samal , Peter De Cat , Ali Esamdin

The extended Main Sequence Turn-off (eMSTO) in the open cluster NGC 2355 is investigated using precise astrometry and photometry from Gaia DR3 and spectroscopic data from the Gaia-ESO Survey. We find a clear positive correlation between the…

太阳与恒星天体物理 · 物理学 2025-11-18 Jayanand Maurya , Yu Zhang , Hubiao Niu
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