1991
DOI: 10.1093/mnras/253.4.683
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On the tidal disruption of a spherical galaxy

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“…10:1). In the last case, tidal tails are generally thin and small, while the same features are more extended and survive for a longer time in major mergers (Namboodiri & Kochhar, 1985).…”
Section: Mass Ratiomentioning
confidence: 92%
“…10:1). In the last case, tidal tails are generally thin and small, while the same features are more extended and survive for a longer time in major mergers (Namboodiri & Kochhar, 1985).…”
Section: Mass Ratiomentioning
confidence: 92%