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pro vyhledávání: '"V. M. Aguirre-Torres"'
We analyse the rotation curves and gravitational stability of a sample of six bulgeless galaxies for which detailed images reveal no evidence for strong bars. We explore two scenarios: Newtonian dark matter models and MOdified Newtonian Dynamics (MON
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::96305789f2353ed3751fbc773b01c736