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Cited by 204

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The initial conditions of star formation in the Ophiuchus main cloud: Kinematics of the protocluster condensations

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André, Ph., Belloche, A., Motte, F., Peretto, N.·2007·Astronomy & Astrophysics

Abstract

Context.The earliest phases of clustered star formation and the origin of the stellar initial mass function (IMF) are currently much debated. In one school of thought the IMF of embedded clusters is entirely determined by turbulent fragmentation at the prestellar stage of star formation, while in a major alternative view it results from dynamical interactions and competitive accretion at the protostellar stage.

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Metadata

Authors
André, P., Belloche, A., Motte, F., & Peretto, N.
Venue
Astronomy & Astrophysics
Publisher
EDP Sciences
Published
2007-06-18
Volume
472
Issue
2
Pages
519-535
ISSN
  • 0004-6361 (ISSN-L)
  • 1432-0746
OpenAlex
W2116528054
Cited by
204
References
0
FWCI
11.07
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: The initial conditions of star formation in the Ophiuchus main cloud: Kinematics of the protocluster condensations. https://app.cochat.ai/papers/10.1051/0004-6361:20077422
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André, P., Belloche, A., Motte, F., & Peretto, N. (2007). The initial conditions of star formation in the Ophiuchus main cloud: Kinematics of the protocluster condensations. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361%3A20077422

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.