H
H. J. G. L. M. Lamers
Researcher at Utrecht University
Publications - 53
Citations - 3574
H. J. G. L. M. Lamers is an academic researcher from Utrecht University. The author has contributed to research in topics: Stars & Galaxy. The author has an hindex of 18, co-authored 53 publications receiving 3363 citations. Previous affiliations of H. J. G. L. M. Lamers include Netherlands Institute for Space Research.
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Mass-loss predictions for O and B stars as a function of metallicity
TL;DR: In this paper, a grid of massive star wind models and mass-loss rates for a wide range of metal abundances between 1=100 Z=Z 10 was calculated and the mass loss rate was shown to be constant in the range between 1/30 Z =Z 3.
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The star cluster population of M 51 - II. Age distribution and relations among the derived parameters
TL;DR: In this paper, the age and mass distribution of star clusters in M51 were found by fitting cluster evolution models to the spectral energy distribution consisting of 8 HST-WFPC2 pass bands.
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The Star Cluster Population of M51: II. Age distribution and relations among the derived parameters
TL;DR: In this paper, the authors used broad-band images from the Hubble Space Telescope (HST) through the near infrared (NICMOS F160W-filter) to study the star cluster population of the interacting spiral galaxy M51 and obtained age, mass, extinction, and effective radius estimates for 1152 star clusters.
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Star cluster formation and disruption time-scales — I. An empirical determination of the disruption time of star clusters in four galaxies
TL;DR: In this article, the authors derived the disruption times of star clusters from cluster samples of four galaxies, M51, M33, the Small Magellanic Cloud (SMC) and the solar neighbourhood.
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Clusters in the inner spiral arms of M 51: The cluster IMF and the formation history
TL;DR: In this paper, an analysis of the HST-WFPC2 observations of the interacting galaxy M51 is presented, where the authors derived their ages, initial masses and extinctions by means of a comparison between spectral energy distribution and the predictions from cluster synthesis models for instantaneous star formation and solar metallicity.