Search Results - "Niederhofer, F"
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Apparent age spreads in clusters and the role of stellar rotation
Published in Monthly notices of the Royal Astronomical Society (21-10-2015)“…We use the Geneva syclist isochrone models that include the effects of stellar rotation to investigate the role that rotation has on the resulting…”
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The search for multiple populations in Magellanic Cloud clusters -- IV. Coeval multiple stellar populations in the young star cluster NGC 1978
Published in Monthly notices of the Royal Astronomical Society (01-07-2018)“…Abstract We have recently shown that the ∼2 Gyr old Large Magellanic Cloud star cluster NGC 1978 hosts multiple populations in terms of star-to-star abundance…”
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The morphology of the sub-giant branch and red clump reveal no sign of age spreads in intermediate-age clusters
Published in Monthly notices of the Royal Astronomical Society (01-04-2015)“…A recent surprise in stellar cluster research, made possible through the precision of Hubble Space Telescope photometry, was that some intermediate-age…”
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The search for multiple populations in Magellanic Cloud clusters – II. The detection of multiple populations in three intermediate-age SMC clusters
Published in Monthly notices of the Royal Astronomical Society (11-03-2017)“…This is the second paper in our series about the search for multiple populations in Magellanic Cloud star clusters using the Hubble Space Telescope. Here we…”
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The search for multiple populations in Magellanic Clouds clusters – V. Correlation between cluster age and abundance spreads
Published in Monthly notices of the Royal Astronomical Society (21-08-2019)“…ABSTRACT In our HST photometric survey, we have been searching for multiple stellar populations (MPs) in Magellanic Clouds (MCs) massive star clusters which…”
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Age as a major factor in the onset of multiple populations in stellar clusters
Published in Monthly notices of the Royal Astronomical Society (01-01-2018)“…It is now well established that globular clusters (GCs) exhibit star-to-star light-element abundance variations (known as multiple populations, MPs). Such…”
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A high fraction of Be stars in young massive clusters: evidence for a large population of near-critically rotating stars
Published in Monthly notices of the Royal Astronomical Society (11-03-2017)“…Recent photometric analyses of the colour-magnitude diagrams of young massive clusters (YMCs) have found evidence for splitting in the main sequence and…”
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The search for multiple populations in Magellanic Cloud clusters – I. Two stellar populations in the Small Magellanic Cloud globular cluster NGC 121
Published in Monthly notices of the Royal Astronomical Society (01-01-2017)“…We started a photometric survey using the WFC3/UVIS instrument onboard the Hubble Space Telescope to search for multiple populations within Magellanic Cloud…”
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The effects of stellar rotation along the main sequence of the 100-Myr-old massive cluster NGC 1850
Published in Monthly notices of the Royal Astronomical Society (01-01-2023)“…ABSTRACT Young star clusters enable us to study the effects of stellar rotation on an ensemble of stars of the same age and across a wide range in stellar mass…”
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The tight subgiant branch of the intermediate-age star cluster NGC 411 implies a single-aged stellar population
Published in Monthly notices of the Royal Astronomical Society (21-09-2016)“…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…”
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Searching for globular cluster chemical anomalies on the main sequence of a young massive cluster
Published in Monthly notices of the Royal Astronomical Society (01-06-2020)“…ABSTRACT The spectroscopic and photometric signals of the star-to-star abundance variations found in globular clusters seem to be correlated with global…”
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Is the escape velocity in star clusters linked to extended star formation histories? Using NGC 7252: W3 as a test case
Published in Monthly notices of the Royal Astronomical Society (21-03-2016)“…The colour–magnitude diagrams of some intermediate-age (1–2 Gyr) star clusters show unexpectedly broad main-sequence turnoffs, raising the possibility that…”
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No evidence for younger stellar generations within the intermediate-age massive clusters NGC 1783, NGC 1806 and NGC 411
Published in Monthly notices of the Royal Astronomical Society (11-07-2016)“…Recently, Li et al. claimed to have found evidence for multiple generations of stars in the intermediate-age clusters NGC 1783, NGC 1806 and NGC 411 in the…”
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A young cluster with an extended main-sequence turnoff: confirmation of a prediction of the stellar rotation scenario
Published in Monthly notices of the Royal Astronomical Society. Letters (21-07-2016)“…We present Hubble Space Telescope photometry of NGC 1850, a ∼100 Myr, ∼105 M⊙ cluster in the Large Magellanic Cloud. The colour–magnitude diagram clearly shows…”
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Spectroscopic detection of multiple populations in the similar to 2 Gyr old cluster Hodge 6 in the LMC
Published in Monthly notices of the Royal Astronomical Society (01-04-2019)“…We report the spectroscopic discovery of abundance spreads (i.e. multiple populations) in the similar to 2 Gyr old cluster in the LMC, Hodge 6. We use…”
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Spectroscopic detection of multiple populations in the ∼2 Gyr old cluster Hodge 6 in the LMC
Published in Monthly notices of the Royal Astronomical Society (21-04-2019)Get full text
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Hubble Space Telescope proper motions of Large Magellanic Cloud star clusters -- I. Catalogues and results for NGC 1850
Published 25-06-2024“…We present proper motion (PM) measurements for a sample of 23 massive star clusters within the Large Magellanic Cloud using multi-epoch data from the Hubble…”
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The VMC survey -- XLVI. Stellar proper motions in the centre of the Large Magellanic Cloud
Published 27-03-2022“…We present proper motion (PM) measurements within the central region of the Large Magellanic Cloud (LMC) using near-infrared data from the VISTA survey of the…”
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Searching for globular cluster chemical anomalies on the main sequence of a young massive cluster
Published 20-04-2020“…The spectroscopic and photometric signals of the star-to-star abundance variations found in globular clusters seem to be correlated with global parameters like…”
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