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Based on new observations with the Wide Field Camera 3 onboard the Hubble Space Telescope, we report the discovery of an extended main sequence turn-off (eMSTO) in the intermediate-age star cluster NGC411. This is the second case of an…

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-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…

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

While the extended main-sequence turn-offs (eMSTOs) found in almost all 1--2 Gyr-old star clusters in the Magellanic Clouds are often explained by postulating extended star-formation histories, the tight subgiant branches (SGBs) seen in…

太阳与恒星天体物理 · 物理学 2016-07-27 Xiaohan Wu , Chengyuan Li , Richard de Grijs , Licai Deng

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

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…

A recent surprise in stellar cluster research, made possible through the precision of Hubble Space Telescope photometry, was that some intermediate age (1-2 Gyr) clusters in the Large and Small Magellanic Clouds have main sequence turn-off…

星系天体物理 · 物理学 2015-06-23 Nate Bastian , Florian Niederhofer

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

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 (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

Most star clusters at an intermediate age (1-2 Gyr) in the Large and Small Magellanic Clouds show a puzzling feature in their color-magnitude diagrams (CMD) that is not in agreement with a simple stellar population. The main sequence…

太阳与恒星天体物理 · 物理学 2016-02-17 F. Niederhofer , N. Bastian , V. Kozhurina-Platais , M. Hilker , S. E. de Mink , I. Cabrera-Ziri , C. Li , B. Ercolano

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 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…

An increasing number of young massive clusters (YMCs) in the Magellanic Clouds have been found to exhibit bimodal or extended main sequences (MSs) in their color--magnitude diagrams (CMDs). These features are usually interpreted in terms of…

太阳与恒星天体物理 · 物理学 2017-08-09 Chengyuan Li , Richard de Grijs , Licai Deng , Antonino P. Milone

The presence of extended main-sequence turn-off (eMSTO) regions in intermediate-age star clusters in the Large and Small Magellanic Clouds is often interpreted as resulting from extended star-formation histories (SFHs), lasting $\geq$ 300…

星系天体物理 · 物理学 2016-07-27 Chengyuan Li , Richard de Grijs , Nathan Bastian , Licai Deng , Florian Niederhofer , Chaoli Zhang

Recent observations of intermediate age (1 - 3 Gyr) massive star clusters in the Large Magellanic Cloud (LMC) have revealed that the majority possess bifurcated or extended main-sequence turn-off (EMSTO) morphologies. This effect can be…

星系天体物理 · 物理学 2015-05-27 Stefan C. Keller , A. Dougal Mackey , Gary S. Da Costa

Extended main sequence turn-offs (eMSTOs) are a common feature in color-magnitude diagrams (CMDs) of young and intermediate-age star clusters in the Magellanic Clouds. The nature of eMSTOs is still debated. The most popular scenarios are…

太阳与恒星天体物理 · 物理学 2018-08-27 Paul Goudfrooij , Leo Girardi , Andrea Bellini , Alessandro Bressan , Matteo Correnti , Guglielmo Costa

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
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