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- aggregation classification "C1".
- aggregation creator B90970.
- aggregation creator person.
- aggregation creator person.
- aggregation creator person.
- aggregation date "2011".
- aggregation format "application/pdf".
- aggregation hasFormat 1843142.bibtex.
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- aggregation isPartOf urn:issn:1824-0178.
- aggregation language "eng".
- aggregation rights "I have transferred the copyright for this publication to the publisher".
- aggregation subject "Physics and Astronomy".
- aggregation title "Global m=1 instabilities and lopsidedness in disc galaxies.".
- aggregation abstract "Lopsidedness is common in spiral galaxies. Often, there is no obvious external cause, such as an interaction with a nearby galaxy, for such features. Alternatively, the lopsidedness may have an internal cause, such as a dynamical instability. In order to explore this idea, we have developed a computer code that searches for self-consistent perturbations in razor-thin disc galaxies and performed a thorough mode-analysis of a suite of dynamical models for disc galaxies embedded in an inert dark matter halo with varying amounts of rotation and radial anisotropy.".
- aggregation authorList BK234566.
- aggregation endPage "132".
- aggregation startPage "127".
- aggregation volume "18".
- aggregation aggregates 1843148.
- aggregation isDescribedBy 1843142.
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