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 H2 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.
Volume 288 -
Accretion Processes in Cosmic Sources (APCS2016) -
ACCRETION ONTO YOUNG STELLAR OBJECTS AND EVOLUTION
H2 shocks and mass accretion rate in high mass young stellar objects (HMYSOs)
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Pre-published on:
March 19, 2018
Published on:
May 16, 2018
Abstract
DOI: https://doi.org/10.22323/1.288.0014
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.