H2 shocks and mass accretion rate in high mass young stellar objects (HMYSOs)

Paolo Persi, Mauricio Tapia
2018 Proceedings of Accretion Processes in Cosmic Sources — PoS(APCS2016)   unpublished
We have observed in the near and mid infrared a sample of high mass young stellar objects in order to understand the mechanisms of formation of these sources. In particular we have searched for the H 2 shocks. From their spectral energy distributions obtained combining observations at different wavelengths, we have obtained the physical parameters such as the mass accretion rate, the disk mass and the luminosity of these source.
doi:10.22323/1.288.0014 fatcat:7edyhua33bg77iq2bswm5usszm