Studying star-forming processes towards G29.862-0.044

AREAL, M. B.; PARON, S.; ORTEGA, M. E.; FARIÑA, C.

Viedma, Río Negro

Congreso; 61a Reunión Anual de la AAA; 2019

Wepresent a multiwavelength study towards the young stellar object(YSO) G29.862-0.044 (hereafter G29), which is embedded in the massivestar-forming region G29.96-0.02, located at a distance of about 6.5kpc.The surrounding interstellar medium of G29 is studied usingmolecular lines data (angular resolution about 15 arcsec)obtained from the databases of the James Clerk Maxwell Telescope. Thephysical conditions of G29 molecularoutflows and the clump where theYSO is embedded are characterized. Near-IR data is also analyzed(spatialresolution of about 0.5 arcsec)obtained with NIRI at Gemini North to have a detailed view of thecircumstellar ambientof G29. The Ks emission towards G29 exhibits acone-like feature pointing to the red molecular outflow. The aimofthis work is to obtain a complete picture of this YSO, the relatedstar-forming processes, and the interstellarmedium around it. Studieslike this are important because they contribute to a comprehensiveunderstanding ofstar formation.p { margin-bottom: 0.25cm; line-height: 115% }