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The Declining Rotation Curve of NGC 157
Published online by Cambridge University Press: 05 March 2013
Abstract
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We have found strong evidence for an abrupt decline in the HI rotation curve of the isolated spiral galaxy NGC 157. Various mass models to account for this, and the implications for the dark matter content of NGC 157, are discussed.
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- Research Article
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- Copyright © Astronomical Society of Australia 1997
References
Ryder, S. D., Zasov, A. V., McIntyre, V. J., Walsh, W., & Sil'chenko, O.
1997, MNRAS, submittedGoogle Scholar
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