Krełowski, J.J.KrełowskiGalazutdinov, G. A.G. A.GalazutdinovMULAS, GiacomoGiacomoMULASBondar, A.A.BondarMusaev, F. A.F. A.MusaevShapovalova, A.A.ShapovalovaCECCHI PESTELLINI, CesareCesareCECCHI PESTELLINIBeletsky, Y.Y.BeletskyLee, B. -C.B. -C.Lee2020-05-192020-05-1920160001-5237http://hdl.handle.net/20.500.12386/24972Using spectra of the star AE Aur (HD 34078), covering the period 1997-2015, we suggest that two strong molecular features of CH and CH<SUP>+</SUP> underwent detectable changes of intensity. In the last five years both CH and CH<SUP>+</SUP> declined sharply and systematically, with the CH/CH<SUP>+</SUP> ratio steadily growing. No variations in the radial velocities of the observed interstellar features was detected during the covered period. <P />STAMPAenVariable Intensities of Molecular Features in the Spectrum of AE AurArticlehttp://acta.astrouw.edu.pl/Vol66/n3/a_66_3_9.html2016AcA....66..391KFIS/05 - ASTRONOMIA E ASTROFISICA