MOSCADELLI, LucaLucaMOSCADELLIGoddi, C.C.GoddiCESARONI, RiccardoRiccardoCESARONIBELTRAN SOROLLA, MARIA TERESAMARIA TERESABELTRAN SOROLLA2022-12-272022-12-272007978-0521-87464-91743-9213http://hdl.handle.net/20.500.12386/32805This work presents the results of VLBI observations of 6.7 GHz methanol and 22.2 GHz water masers towards the mm core A in the massive star-forming region G24.78+0.08. Comparing the maser with previous millimeter interferometric and recent continuum VLA observations, the physical properties and the gas kinematics of the G24 A core on linear scales from ~100 AU to ~0.1 pc are determined.ELETTRONICOenMassive star-formation in G24.78+0.08 studied by means of maser VLBI and thermal interferometric observationsConference paper10.1017/S17439213070126902-s2.0-38849199686https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/massive-starformation-in-g2478008-studied-by-means-of-maser-vlbi-and-thermal-interferometric-observations/FF42B4B69ACF87694973558C7EC2B9CChttps://api.elsevier.com/content/abstract/scopus_id/388491996862007IAUS..242..135MFIS/05 - ASTRONOMIA E ASTROFISICA