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SONYC - Substellar Objects in Nearby Young Clusters - is a survey program to investigate the frequency and properties of brown dwarfs down to masses below the Deuterium burning limit in nearby star fo...
Although the stellar and substellar populations have been studied in various young and old open clusters, additional studies in clusters in the age range from 5 to 100Myr is crucial (e.g. to give more...
Accretion disks in white dwarf systems are believed to be tilted. In a recent publication, the lift force has been suggested to be a source to disk tilt, a source that is likely relevant to all accret...
In this work, we derive the stellar initial mass function (IMF) from the superposition of mass distributions of dense cores, generated through gravoturbulent fragmentation of unstable clumps in molecu...
Substellar binarity among nearby white dwarfs。
Lambda Orionis Star Forming Region:toward a comprehensive study of the stellar and substellar population。
A CCD Search for Wide Metal-Poor Binary Stars:Approaching the Metal-Depleted Substellar Limit。
An empirical criterion to classify T Tauri stars and substellar analogs using low-resolution spectroscopy。
Substellar secondaries in zero-age cataclysmic variables。

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