We adopt the deep learning method CASI-3D (Convolutional Approach to Structure Identification-3D) infer orientation of magnetic fields in sub-/trans- Alfvenic turbulent clouds from molecular line emission. carry out magnetohydrodynamic simulations with different field strengths and use these generate synthetic observations. apply 3D radiation transfer code RADMC-3d model 12CO 13CO (J = 1-0) emi...

We present 12CO (J=2-1) sensitive molecular line and 1.3 mm continuum observations made with the Submillimeter Array (SMA) of bipolar outflow associated young star located in Bok globule known as CB 26. The SMA were carried out its extended configuration allowing us to study kinematics structure about 1 arcsec or 140 au resolution. find that dusty edge-on circumstellar disk related has an proje...

ABSTRACT The velocity gradients technique (VGT) and the probability density functions (PDFs) of mass are tools to study turbulence, magnetic fields, self-gravity in molecular clouds. However, self-absorption can significantly make observed intensity different from column structures. In this work, we effects on VGT PDFs utilizing three synthetic emission lines CO isotopologues 12CO (1–0), 13CO C...