BELTRAN SOROLLA, MARIA TERESAMARIA TERESABELTRAN SOROLLA2020-06-192020-06-1920150004-640Xhttp://hdl.handle.net/20.500.12386/26159Intermediate-mass protostars are the long-forgotten actors in the star-formation scenario. Historically, intermediate-mass stars have been associated to the low-mass regime and not too much attention has been drawn to them as a separate group. However, although their pre-main sequence evolution should be similar to that of low-mass protostars, intermediate-mass young stellar objects share many characteristics with their higher mass counterparts. This suggests that the star-formation mechanism could be similar for all luminosities.STAMPAenArticle10.1007/s10509-014-2151-02-s2.0-84925538812000350206600009https://link.springer.com/article/10.1007%2Fs10509-014-2151-02015Ap&SS.355..283BFIS/05 - ASTRONOMIA E ASTROFISICAScienze Fisiche Settori ERC (ERC) di riferimento::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_4 Formation of stars and planets