Our understanding of complex organic chemistry during the formation of stars and planets is shaped by a handful of cherry-picked sources with bright molecular emission lines. This observational bias impedes our assessment of how universal chemical complexity is during star formation. The lack of systematic wideband spe...
M. Drozdovskaya, T. Csengeri, Maria Teresa Beltrán et al.· 0 citations
The interstellar medium (ISM) is magnetized at all scales and phases in our Galaxy and other galaxies across the Universe. Spectro-polarimetric millimetre observations are essential to probe the role of the interstellar magnetic fields in the dynamics of the cold universe, and how this affects the star formation proces...
J. Girart, G. Fuller, W. Vlemmings et al.· 0 citations
Existing sub-mm observatories such as ALMA have provided statistics on the planet-forming mass reservoirs within circumstellar disks around stars in stellar clusters out to distances of $\sim$400pc. However, these disks are not where most planets form. Many stars, and hence planets, form in more massive clusters, which...
Thomas J. Haworth, G. Rosotti, C. Manara et al.· 0 citations
How does a star's birth environment set the mass, angular momentum and chemical complexity delivered to its planet-forming disk, and thereby whether it builds planets, brown dwarfs or stellar companions? This requires following material from the cloud to the sub-au to few-au scales where infalling gas, magnetized winds...
M. Kuffmeier, J. Pineda, P. Schilke et al.· 0 citations
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