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Cited by 160

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Fragmentation of Molecular Clouds: The Initial Phase of a Stellar Cluster

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Klessen, Ralf S., Burkert, Andreas, Bate, Matthew R.·1998·The Astrophysical Journal

Abstract

The isothermal gravitational collapse and fragmentation of a region within a molecular cloud and the subsequent formation of a protostellar cluster are investigated numerically. The clump mass spectrum that forms during the fragmentation phase can be well approximated by a power-law distribution dN / dM ∝ M −1.5 . In contrast, the mass spectrum of protostellar cores that form in the centers of Jeans-unstable clumps and that evolve through accretion and N -body interactions is described by a lognormal distribution with a width that is in excellent agreement with observations of multiple stellar systems.

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Metadata

Authors
Klessen, R. S., Burkert, A., & Bate, M. R.
Venue
The Astrophysical Journal
Published
1998-07-10
Volume
501
Issue
2
Pages
L205-L208
ISSN
0004-637X (ISSN-L)
OpenAlex
W2004460878
Cited by
160
References
0
FWCI
9.61
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Fragmentation of Molecular Clouds: The Initial Phase of a Stellar Cluster. https://app.cochat.ai/papers/10.1086/311471
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Klessen, R. S., Burkert, A., & Bate, M. R. (1998). Fragmentation of Molecular Clouds: The Initial Phase of a Stellar Cluster. The Astrophysical Journal. https://doi.org/10.1086/311471

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