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• W3100647185 startingPage "991" @default.
• W3100647185 abstract "The evolution of a stellar bar transforms not only the galactic disc, but also the host dark matter halo. We present high-resolution, fully self-consistent N-body simulations that clearly demonstrate that dark matter halo central density cusps flatten as the bar torques the halo. This effect is independent of the bar formation mode and occurs even for rather short bars. The halo and bar evolution is mediated by resonant interactions between orbits in the halo and the bar pattern speed, as predicted by linear Hamiltonian perturbation theory. The bar lengthens and slows as it loses angular momentum, a process that occurs even in rather warm discs. We demonstrate that the bar and halo response can be critically underestimated for experiments that are unable to resolve the relevant resonant dynamics; this occurs when the phase space in the resonant region is undersampled or plagued by noise." @default.
• W3100647185 created "2020-11-23" @default.
• W3100647185 creator A5006709063 @default.
• W3100647185 creator A5036640448 @default.
• W3100647185 creator A5064379623 @default.
• W3100647185 date "2005-11-01" @default.
• W3100647185 modified "2023-09-29" @default.
• W3100647185 title "Bar-induced evolution of dark matter cusps" @default.
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• W3100647185 cites W1671770934 @default.
• W3100647185 cites W1964280853 @default.
• W3100647185 cites W1966665981 @default.
• W3100647185 cites W1968638976 @default.
• W3100647185 cites W1970381301 @default.
• W3100647185 cites W1971152913 @default.
• W3100647185 cites W1981333407 @default.
• W3100647185 cites W1985631297 @default.
• W3100647185 cites W1994405258 @default.
• W3100647185 cites W1996072085 @default.
• W3100647185 cites W2003092390 @default.
• W3100647185 cites W2008214685 @default.
• W3100647185 cites W2009083897 @default.
• W3100647185 cites W2009473892 @default.
• W3100647185 cites W2010017913 @default.
• W3100647185 cites W2010581546 @default.
• W3100647185 cites W2013525260 @default.
• W3100647185 cites W2014420597 @default.
• W3100647185 cites W2014592430 @default.
• W3100647185 cites W2018350350 @default.
• W3100647185 cites W2021474968 @default.
• W3100647185 cites W2023344562 @default.
• W3100647185 cites W2023428467 @default.
• W3100647185 cites W2023528546 @default.
• W3100647185 cites W2030520011 @default.
• W3100647185 cites W2032357316 @default.
• W3100647185 cites W2032772536 @default.
• W3100647185 cites W2033180045 @default.
• W3100647185 cites W2034040738 @default.
• W3100647185 cites W2034241156 @default.
• W3100647185 cites W2035547408 @default.
• W3100647185 cites W2036635689 @default.
• W3100647185 cites W2041131158 @default.
• W3100647185 cites W2042904965 @default.
• W3100647185 cites W2043137394 @default.
• W3100647185 cites W2047159064 @default.
• W3100647185 cites W2047843291 @default.
• W3100647185 cites W2050114676 @default.
• W3100647185 cites W2052986856 @default.
• W3100647185 cites W2057139020 @default.
• W3100647185 cites W2057462968 @default.
• W3100647185 cites W2057877481 @default.
• W3100647185 cites W2060638494 @default.
• W3100647185 cites W2063096789 @default.
• W3100647185 cites W2065980009 @default.
• W3100647185 cites W2075280515 @default.
• W3100647185 cites W2077334492 @default.
• W3100647185 cites W2082012530 @default.
• W3100647185 cites W2083034637 @default.
• W3100647185 cites W2083950714 @default.
• W3100647185 cites W2086882315 @default.
• W3100647185 cites W2087481460 @default.
• W3100647185 cites W2090004102 @default.
• W3100647185 cites W2098893665 @default.
• W3100647185 cites W2132377084 @default.
• W3100647185 cites W2138946832 @default.
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• W3100647185 cites W2161078062 @default.
• W3100647185 cites W2163075131 @default.
• W3100647185 cites W2164797599 @default.
• W3100647185 cites W2170991355 @default.
• W3100647185 cites W2171582647 @default.
• W3100647185 cites W2949915762 @default.
• W3100647185 cites W3098339996 @default.
• W3100647185 cites W3098779512 @default.
• W3100647185 cites W3099312230 @default.
• W3100647185 cites W3100118165 @default.
• W3100647185 cites W3100234948 @default.
• W3100647185 cites W3100618087 @default.
• W3100647185 cites W3101290424 @default.
• W3100647185 cites W3101894563 @default.
• W3100647185 cites W3102652355 @default.
• W3100647185 cites W3102706962 @default.
• W3100647185 cites W3102981450 @default.
• W3100647185 cites W3103162296 @default.
• W3100647185 cites W3103502977 @default.
• W3100647185 cites W3103772912 @default.
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• W3100647185 doi "https://doi.org/10.1111/j.1365-2966.2005.09501.x" @default.
• W3100647185 hasPublicationYear "2005" @default.
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