5 papers
Characterising magnetic fields at the onset of star cluster formation: From giant molecular clouds to infrared dark clumps
Ria Ramkumar, Nicolas Peretto, Gary A. Fuller +2
The role of magnetic fields in the observed inefficiency of star formation in Galactic molecular clouds is a widely debated topic, with the past decade seeing an explosion of obser…
Destructuring the disk of AB Aurigae: Dynamics and accretion
Anthony Boccaletti, Emmanuel Di Folco, Anne Dutrey +23
In this paper, we present near-IR polarized images of the AB Aur disk at three epochs spanning 3.85 years with SPHERE/IRDIS, as well as Halpha images obtained with SPHERE/ZIMPOL at…
Can Clump Properties Predict Core Distribution in Star Formation? A Statistical Analysis of MHD Simulations
Wei-An Chen, Seamus D. Clarke, Ya-Wen Tang
Dense cores, the progenitors of stars, are in sub-pc scale and fragmented from pc-scale clumps. However, it is still unclear that how strongly the fragmentation process is affected…
A Tale of Three: Magnetic Fields along the Orion Integral-Shaped Filament as Revealed by JCMT BISTRO survey
Jintai Wu, Keping Qiu, Frederick Poidevin +152
As part of the BISTRO survey, we present JCMT 850 m polarimetric observations towards the Orion Integral-Shaped Filament (ISF) that covers three portions known as OMC-1, OMC-2,…
Alignment Parameters: Quantifying Dense Core Alignment in Star-forming Regions
Wei-An Chen, Ya-Wen Tang, Seamus D. Clarke
Recent high-resolution observations at millimeter (mm) and sub-mm reveal a diverse spatial distribution for sub-pc scale dense cores within star-forming regions, ranging from clust…