Complex Organic Molecules (COMs), such as propylene (CH3CHCH2) and the isomers of C2H4O2 are detected in cold molecular clouds (such as TMC-1) with high fractional abundances (Marcelino et al., Astrophys. J., 2007, 665, L127). The formation mechanism for these species is the subject of intense speculation, as is the possibility of the formation of simple amino acids such as glycine (NH2CH2COOH)...

Abstract The Large Magellanic Cloud (LMC) is the nearest laboratory for detailed studies on formation and survival of complex organic molecules (COMs), including biologically important ones, in low-metallicity environments—typical earlier cosmological epochs. We report results 1.2 mm continuum molecular line observations three fields star-forming region N 105 with Atacama Millimeter/submillimet...

Current 3D reconstruction methods using stereo vision can produce good results, but they tend to yield very sparse outputs and suffer from several challenges. One of them is the well-known correspondence problem, whereby similar features in different images are often too ambiguous to match reliably. The problem is accentuated when the object being scanned is textureless. Under these circumstanc...