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Cited by 320

The DOI matches its Crossref record; 13 of the 13 references it cites were found in a registry or an index.

Bar-Halo Interaction and Bar Growth

Open access
Athanassoula, E.·2002·The Astrophysical Journal

Abstract

I show that strong bars can grow in galactic disks, even when the latter are immersed in halos whose mass within the disk radius is comparable to, or larger than, the mass of the disk. I argue that this is due to the response of the halo and in particular to the destabilizing influence of the halo resonant stars. Via this instability mechanism, the halo can stimulate, rather than restrain, the growth of the bar.

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Metadata

Authors
Athanassoula, E.
Venue
The Astrophysical Journal
Published
2002-04-20
Volume
569
Issue
2
Pages
L83-L86
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2162945864
Cited by
320
References
13
FWCI
11.64
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Bar-Halo Interaction and Bar Growth. https://app.cochat.ai/papers/10.1086/340784
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Athanassoula, E. (2002). Bar-Halo Interaction and Bar Growth. The Astrophysical Journal. https://doi.org/10.1086/340784

Data sources

Bibliographic data: Semantic Scholar, OpenAlex, Crossref.

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.