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Journal ArticleDOI

Modeling of the Initial Mass Function Using the Metropolis−Hastings Algorithm

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TLDR
In this article, a stochastic model for the hierarchical fragmentation of a molecular cloud was developed, where the number of fragments, time between successive fragmentation steps, and mass of a fragment were considered as random variables, and fragment masses were generated using the Metropolis-Hastings algorithm.
Abstract
A stochastic model has been developed for the hierarchical fragmentation of a molecular cloud. Here, the number of fragments, time between successive fragmentation steps, and mass of a fragment are considered as random variables, and fragment masses are generated using the Metropolis-Hastings algorithm. The resulting mass spectra, computed at different projected distances and taking opacity into consideration, show a signature of mass segregation. The critical mass, mass spectrum, and mass segregation are consistent with the observations of young massive clusters in our Galaxy as well as in external galaxies.

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Citations
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Journal ArticleDOI

The initial mass function modeled by a left truncated beta distribution

TL;DR: In this article, a left truncated beta probability density function was introduced to demonstrate the advantage of introducing a four-parameter initial mass function for the stars and the presence of brown dwarfs.
Journal ArticleDOI

Cosmic history of integrated galactic stellar initial mass function : a simulation study

TL;DR: In this paper, the authors investigated the effect of the evolution of the stellar initial mass function (IMF) with increasing redshift on the formation of massive clusters in star burst galaxies.
Journal ArticleDOI

Cosmic History of the Integrated Galactic Stellar Initial Mass Function: A Simulation Study

TL;DR: In this article, the authors investigate the evolution of the stellar initial mass function (IMF) and varying indices of β for the integrated galactic initial mass functions, in relation to several measures of star formation rates of galaxies at various redshifts by random simulation.
Journal ArticleDOI

The low-mass Initial Mass Function in the 30 Doradus starburst cluster

TL;DR: In this article, the authors presented deep Hubble Space Telescope (HST) NICMOS 2 F160W band observations of the central 56*57" (14pc*14.25pc) region around R136 in the starburst cluster 30 Dor (NGC 2070) located in the Large Magellanic Cloud.
Journal Article

The Formation and Early Dynamical Evolution of Bound Stellar Systems

TL;DR: In this paper, the results of numerical N-body calculations which simulate the dynamical evolution of young clusters as they emerge from molecular clouds have been presented, and the combination of these parameters which result in the production of bound stellar groups after the gas not used in star formation is completely dispersed.
References
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Journal ArticleDOI

No evidence of mass segregation in massive young clusters

TL;DR: In this article, the authors investigate the validity of the mass segregation indicators commonly used in analysing young stellar clusters and find that commonly used indicators are highly sensitive to sample incompleteness in observational data and that radial completeness determinations do not provide satisfactory corrections.
Journal ArticleDOI

On the formation rate of galactic clusters in clouds of various masses

TL;DR: In this article, the formation of a bound cluster depends on the efficiency of star formation in the cloud, and this efficiency depended on the relative mass of stars that have formed by the time a sufficiently luminous star destroys the cloud.
Journal ArticleDOI

No evidence for mass segregation in massive young clusters

TL;DR: In this paper, the authors investigate the validity of the mass segregation indicators commonly used in analysing young stellar clusters and find that commonly used indicators are highly sensitive to sample incompleteness in observational data and that radial completeness determinations do not provide satisfactory corrections.
Journal ArticleDOI

The lower mass function of the young open cluster Blanco 1: from 30 Mjup to 3 Mo

TL;DR: In this paper, the authors performed a deep wide field optical survey of the young (~100-150 Myr) open cluster Blanco1 to study its low mass population well down into the brown dwarf regime and estimate its mass function over the whole cluster mass range.
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