Chekhonadskikh, F. A.2014-03-132014-03-132010Odessa Astronomical Publicationshttps://dspace.onu.edu.ua/handle/123456789/4595Odessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 07/2010 . – Vol.23.The results of the spectroscopic researches of classical Chepheids of the Magellanic Clouds (MC) are presented in this paper. 21 spectra for the Large Magellanic Cloud (LMC) and 10 for the Small Magellanic Cloud (SMC) were investigated. I obtained highly accurate values of e ective temperatures (Teff ), of the logarithm of the surface gravity(log g), of the microturbulence velocity (Vt), of abundances of elements for all of the objects. There is a good agreement with previous studies, some data were obtained for the rst time.enClassical Cepheids: parameters of stellar athmosphereMagellanic Clouds: abundancesArticle