MASSI, FabrizioFabrizioMASSIMOSCADELLI, LucaLucaMOSCADELLIARCIDIACONO, CARMELOCARMELOARCIDIACONOBACCIOTTI, FrancescaFrancescaBACCIOTTI2020-11-252020-11-252018978-11071924541743-9213http://hdl.handle.net/20.500.12386/28528Whether high-mass stars (M > 7M☉) emerge from a scaled-up version of the low-mass star formation scenario, i. e. through disk-mediated accretion, is still debated. We present the first results of an observational programme aimed to map the innermost regions of high-mass stellar objects by combining together high-spatial resolution maser and radio continuum observations, and near-infrared imaging.STAMPAenConference paper10.1017/S1743921317011644https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/innermost-regions-of-massive-protostars-traced-by-masers-highresolution-radio-continuum-and-nearinfrared-imaging/2ED76FA59B3094D4A5B52E99DD988CAB2018IAUS..336..289MFIS/05 - ASTRONOMIA E ASTROFISICA