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of the gaseous disk |
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|
|
|
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Between spiral |
|
|
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In Spiral |
|
stability |
|
|
|
symmetric gravitational potential |
may be shifted relative to density exterema |
may be shifted relative to density exterema |
References: Lyakhovich V.V., Fridman A.M., Khoruzhii O.V., Astronomy Reports, Vol.40, No.1,pp.18-28. Translation from Astronomicheskii Zhurnal, Vol.73, No.1,pp.24-35, 1996.
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