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The GUAPOS project: G31.41+0.31 Unbiased ALMA sPectral Observational Survey -- I. Isomers of CHO
C. Mininni, M. T. Beltrán, V. M. Rivilla +10
Understanding the degree of chemical complexity that can be reached in star-forming regions, together with the identification of precursors of the building blocks of life in the in…
Binary system and jet precession and expansion in G35.20-0.74N
M. T. Beltrán, R. Cesaroni, L. Moscadelli +3
Context. ALMA observations of the high-mass star-forming region G35.20-0.74N have revealed the presence of a Keplerian disk in core B rotating about a massive object of 18 Msun, as…
SiO collimated outflows driven by high-mass YSOs in G24.78+0.08
C. Codella, M. T. Beltran, R. Cesaroni +4
We imaged the molecular outflows towards the cluster of high-mass young stellar objects G24.78+0.08 at high-angular resolution using SiO emission, which is considered the classical…
Dissecting a hot molecular core: The case of G31.41+0.31
R. Cesaroni, M. T. Beltrán, Q. Zhang +2
We made a detailed observational analysis of a well known hot molecular core lying in the high-mass star-forming region G31.41+0.31. This core is believed to contain deeply embedde…
On the kinematics of massive star forming regions: the case of IRAS 17233-3606
S. Leurini, C. Codella, L. Zapata +3
Direct observations of accretion disks around high-mass young stellar objects would help to discriminate between different models of formation of massive stars. However, given the…
Infall, outflow, and rotation in the G19.61-0.23 hot molecular core
R. S. Furuya, R. Cesaroni, H. Shinnaga
Aims: The main goal of this study is to perform a sub-arcsecond resolution analysis of the high-mass star formation region G19.61-0.23, both in the continuum and molecular line emi…