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相关论文: Multiple stellar populations in Magellanic Cloud c…

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The split main sequences (MSs) and extended MS turnoffs (eMSTOs) detected in a few young clusters have demonstrated that these stellar systems host multiple populations differing in a number of properties such as rotation and, possibly,…

Nearly all the star clusters with ages of ~1-2 Gyr in both Magellanic Clouds exhibit an extended main-sequence turn off (eMSTO) whose origin is under debate. The main scenarios suggest that the eMSTO could be either due to multiple…

太阳与恒星天体物理 · 物理学 2016-03-23 A. P. Milone , A. F. Marino , F. D'Antona , L. R. Bedin , G. S. Da Costa , H. Jerjen , A. D. Mackey

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

Young and intermediate-age star clusters of both Magellanic Clouds exhibit complex color-magnitude diagrams. In addition to the extended main-sequence turn-offs (eMSTOs), commonly observed in star clusters younger than ~2 Gyr, the clusters…

We present a spectroscopic analysis of main sequence (MS) stars in the young globular cluster NGC1818 (age~40 Myrs) in the Large Magellanic Cloud. Our photometric survey on Magellanic Clouds clusters has revealed that NGC1818, similarly to…

太阳与恒星天体物理 · 物理学 2018-08-29 A. F. Marino , N. Przybilla , A. P. Milone , G. Da Costa , F. D'Antona , A. Dotter , A. Dupree

By far, the color-magnitude diagrams (CMDs) of Galactic open clusters have been considered proto-types of single stellar populations. By using photometry in ultraviolet and optical bands we discovered that the nearby young cluster NGC6705…

太阳与恒星天体物理 · 物理学 2018-08-29 A. F. Marino , A. P. Milone , L. Casagrande , N. Przybilla , L. Balaguer-Nunez , M. Di Criscienzo , A. Serenelli , F. Vilardell

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

A large number of intermediate-age (~1-2-Gyr old) globular clusters (GCs) in the Large and the Small Magellanic Cloud (MC) exhibit either bimodal or extended main-sequence (MS) turn off and dual red clump. Moreover, recent papers have shown…

太阳与恒星天体物理 · 物理学 2015-11-04 A. P. Milone

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)…

太阳与恒星天体物理 · 物理学 2017-01-18 Matteo Correnti , Paul Goudfrooij , Andrea Bellini , Jason S. Kalirai , Thomas H. Puzia

In the past years, we have undertaken an extensive investigation of LMC and SMC star clusters based on HST data. We present photometry and astrometry of stars in 101 fields observed with the WFC/ACS, UVIS/WFC3 and NIR/WFC3 cameras. These…

The discovery of multiple MSs in NGC2808 and Omega Centauri, and multiple SGBs in NGC1851 and NGC6388 has challenged the long-held paradigm that GCs consist of simple stellar populations. This picture has been further complicated by recent…

天体物理学 · 物理学 2009-11-13 A. P. Milone , L. R. Bedin , G. Piotto , J. Anderson

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

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

The color-magnitude diagrams (CMDs) of young star clusters show that, particularly at ultraviolet wavelengths, their upper main sequences (MSs) bifurcate into a sequence comprising the bulk population and a blue periphery. The spatial…

太阳与恒星天体物理 · 物理学 2021-05-12 Yujiao Yang , Chengyuan Li , Richard de Grijs , Licai Deng

We discuss new photometry from high-resolution images of 7 intermediate-age (1-2 Gyr) star clusters in the Large Magellanic Cloud taken with the Advanced Camera for Surveys on board the Hubble Space Telescope. We fit color-magnitude…

太阳与恒星天体物理 · 物理学 2015-05-28 Paul Goudfrooij , Thomas H. Puzia , Vera Kozhurina-Platais , Rupali Chandar

We used a combination of optical and near-UV Hubble Space Telescope photometry and FLAMES/ESO-VLT high-resolution spectroscopy to characterize the stellar content of the old and massive globular cluster (GC) NGC121 in the Small Magellanic…

太阳与恒星天体物理 · 物理学 2016-10-05 E. Dalessandro , E. Lapenna , A. Mucciarelli , L. Origlia , F. R. Ferraro , B. Lanzoni

Nearly all star clusters younger than ~600 Myr exhibit extended main sequence turn offs and split main sequences (MSs) in their color-magnitude diagrams. Works based on both photometry and spectroscopy have firmly demonstrated that the red…

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…

Recent discoveries of bimodal main sequences (MSs) associated with young clusters (with ages $\lesssim 1$ Gyr) in the Magellanic Clouds have drawn a lot of attention. One of the prevailing formation scenarios attributes these split MSs to a…

太阳与恒星天体物理 · 物理学 2018-06-05 Yujiao Yang , Chengyuan Li , Licai Deng , Richard de Grijs , Antonino P. Milone

The Magellanic Clouds host a large population of massive (> 10^4 Msun) star clusters with ages ranging from a few Myr to 12 Gyr. In nearly all cases, close inspection of their CMDs reveals features that deviate from expectations of a…

星系天体物理 · 物理学 2017-11-06 I. Cabrera-Ziri , S. Martocchia , K. Hollyhead , N. Bastian
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