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The document presents an analytical approach to ram pressure stripping of galaxies, focusing on the kinematic description of gas removal due to interactions with the intracluster medium (ICM). It establishes two asymptotic limits for the stripping process based on the duration of the ram pressure pulse, correlating it with the Gunn & Gott criterion for longer pulses and a momentum transfer approach for shorter pulses. The findings are validated against SPH simulations and applied to a sample of Virgo galaxi

Author

Oscar Villanueva

Language

EN