Low-column-density filaments align parallel to magnetic fields while high-column-density wide filaments align perpendicular, with transition at roughly 0.8-8 x 10^21 cm^-2; projection effects analyzed statistically.
Low Mass Star Formation in the Taurus-Auriga Clouds
2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
abstract
We review the history and structure of star formation in the Taurus-Auriga dark clouds. Our discussion includes a summary of the macroscopic cloud properties, the population of single and binary pre-main sequence stars, the properties of jets and outflows, and detailed summaries of selected individual objects. We include comprehensive tables of dark clouds, young stars, and jets in the clouds.
years
2026 2verdicts
UNVERDICTED 2representative citing papers
SKA-Mid Band 5b continuum observations at 12.5 GHz will resolve disk substructures at ~0.05 arcsec to investigate their origin and role in planet assembly.
citing papers explorer
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Statistical analysis of the relative orientations between filaments and magnetic fields using Herschel and Planck data in star-forming regions
Low-column-density filaments align parallel to magnetic fields while high-column-density wide filaments align perpendicular, with transition at roughly 0.8-8 x 10^21 cm^-2; projection effects analyzed statistically.
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Substructures in Planet-Forming Disks with the SKAO
SKA-Mid Band 5b continuum observations at 12.5 GHz will resolve disk substructures at ~0.05 arcsec to investigate their origin and role in planet assembly.