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Star cluster disruption by giant molecular clouds

Monthly notices of the Royal Astronomical Society, 2006-09, Vol.371 (2), p.793-804

2006

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Disruption time scales of star clusters in different galaxies

Astronomy and astrophysics (Berlin), 2005-01, Vol.429 (1), p.173-179

2005

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Early disc accretion as the origin of abundance anomalies in globular clusters

Monthly notices of the Royal Astronomical Society, 2013-12, Vol.436 (3), p.2398-2411

2013

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Clusters in the solar neighbourhood: how are they destroyed?

Astronomy and astrophysics (Berlin), 2006-08, Vol.455 (2), p.L17-L20

2006

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Mass-loss predictions for O and B stars as a function of metallicity

Astronomy and astrophysics (Berlin), 2001-04, Vol.369 (2), p.574-588

2001

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An analytical description of the disruption of star clusters in tidal fields with an application to Galactic open clusters

Astronomy and astrophysics (Berlin), 2005-10, Vol.441 (1), p.117-129

2005

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The initial mass distribution of the M82 star cluster system

Monthly notices of the Royal Astronomical Society, 2005-12, Vol.364 (3), p.1054-1062

2005

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Systematic uncertainties in the analysis of star cluster parameters based on broad-band imaging observations

Monthly notices of the Royal Astronomical Society, 2005-05, Vol.359 (3), p.874-894

2005

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Evidence for environmentally dependent cluster disruption in M83

Monthly notices of the Royal Astronomical Society, 2011-10, Vol.417 (1), p.L6-L10

2011

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The star cluster population of M 51. II. Age distribution and relations among the derived parameters

Astronomy and astrophysics (Berlin), 2005-03, Vol.431 (3), p.905-924

2005

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ACS imaging of star clusters in M 51 : I. Identification and radius distribution

Astronomy and astrophysics (Berlin), 2007-07, Vol.469 (3), p.925-940

2007

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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

Monthly notices of the Royal Astronomical Society, 2003-01, Vol.338 (3), p.717-732

2003

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The difference in metallicity distribution functions of halo stars and globular clusters as a function of galaxy type

Astronomy and astrophysics (Berlin), 2017-10, Vol.606

2017

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The spatial distribution of star and cluster formation in M 51

Astronomy and astrophysics (Berlin), 2009-01, Vol.494 (1), p.81-93

2009

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Observational evidence for a truncation of the star cluster initial mass function at the high mass end

Astronomy and astrophysics (Berlin), 2006-02, Vol.446 (2), p.L9-L12

2006

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The star cluster population of m 51. III. Cluster disruption and formation history

Astronomy and astrophysics (Berlin), 2005-10, Vol.441 (3), p.949-960

2005

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The photometric evolution of star clusters and the preferential loss of low-mass bodies – with an application to globular clusters

Astronomy and astrophysics (Berlin), 2008-10, Vol.490 (1), p.151-171

2008

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The photometric evolution of dissolving star clusters: II. Realistic models. Colours and M/L ratios

Astronomy and astrophysics (Berlin), 2009-08, Vol.502 (3), p.817-832

2009

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On the nature of pre-main sequence candidate stars in the Large Magellanic Cloud

Astronomy and astrophysics (Berlin), 2005-03, Vol.432 (2), p.619-632

2005

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The remarkable light and colour variability of Small Magellanic Cloud Be stars

Astronomy and astrophysics (Berlin), 2006-09, Vol.456 (3), p.1027-1035

2006

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The mass-loss rates of Wolf–Rayet stars explained by optically thick radiation driven wind models

Astronomy and astrophysics (Berlin), 2002-07, Vol.389 (1), p.162-179

2002

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The early evolution of young massive clusters: The kinematic history of NGC 6611/M16

Astronomy and astrophysics (Berlin), 2023-02, Vol.670, p.A108

2023

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The difference in metallicity distribution functions of halo stars and globular clusters as a function of galaxy type: A tracer of globular cluster formation and evolution

Astronomy and astrophysics (Berlin), 2017-10, Vol.606, p.A85

2017

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ACS imaging of star clusters in M51 II. The luminosity function and mass function across the disk

Astronomy and astrophysics (Berlin), 2008-09, Vol.487 (3), p.937-949

2008

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A study of the expanding envelope of Nova V1974 Cyg 1992 based on IUE high resolution spectroscopy

Astronomy and astrophysics (Berlin), 2004-06, Vol.420 (2), p.571-588

2004

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Star cluster disruption by giant molecular clouds

Disruption time scales of star clusters in different galaxies

Early disc accretion as the origin of abundance anomalies in globular clusters

Clusters in the solar neighbourhood: how are they destroyed?

Mass-loss predictions for O and B stars as a function of metallicity

An analytical description of the disruption of star clusters in tidal fields with an application to Galactic open clusters

The initial mass distribution of the M82 star cluster system

Systematic uncertainties in the analysis of star cluster parameters based on broad-band imaging observations

Evidence for environmentally dependent cluster disruption in M83

The star cluster population of M 51. II. Age distribution and relations among the derived parameters

ACS imaging of star clusters in M 51 : I. Identification and radius distribution

Star cluster formation and disruption time-scales — I. An empirical determination of the disruption time of star clusters in four galaxies

The difference in metallicity distribution functions of halo stars and globular clusters as a function of galaxy type

The spatial distribution of star and cluster formation in M 51

Observational evidence for a truncation of the star cluster initial mass function at the high mass end

The star cluster population of m 51. III. Cluster disruption and formation history

The photometric evolution of star clusters and the preferential loss of low-mass bodies – with an application to globular clusters

The photometric evolution of dissolving star clusters: II. Realistic models. Colours and M/L ratios

On the nature of pre-main sequence candidate stars in the Large Magellanic Cloud

The remarkable light and colour variability of Small Magellanic Cloud Be stars

The mass-loss rates of Wolf–Rayet stars explained by optically thick radiation driven wind models

The early evolution of young massive clusters: The kinematic history of NGC 6611/M16

The difference in metallicity distribution functions of halo stars and globular clusters as a function of galaxy type: A tracer of globular cluster formation and evolution

ACS imaging of star clusters in M51 II. The luminosity function and mass function across the disk

A study of the expanding envelope of Nova V1974 Cyg 1992 based on IUE high resolution spectroscopy

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