Li, J. J.J. J.LiMOSCADELLI, LucaLucaMOSCADELLICESARONI, RiccardoRiccardoCESARONIFuruya, R. S.R. S.FuruyaXu, Y.Y.XuUsuda, T.T.UsudaMenten, K. M.K. M.MentenPestalozzi, M.M.PestalozziELIA, Davide QuintinoDavide QuintinoELIASCHISANO, EUGENIOEUGENIOSCHISANO2022-12-202022-12-20201297811070328421743-9213http://hdl.handle.net/20.500.12386/32792We investigated the high-mass star-forming region G28.87+0.07 by means of maser kinematics, including H<SUB>2</SUB>O, CH<SUB>3</SUB>OH, and OH, and radio to infrared, continuum observations. All observational evidence suggests that these masers are associated with the same young star of 20-30 M<SUB>⊙</SUB>, still in the main accretion phase and surrounded by a rich stellar cluster.ELETTRONICOenConference paper10.1017/S17439213120068982-s2.0-84864429912https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/massive-starformation-toward-g2887007/7655978F455BC30124895E5EE7C4282Bhttps://api.elsevier.com/content/abstract/scopus_id/848644299122012IAUS..287..180LFIS/05 - ASTRONOMIA E ASTROFISICA