Magnetic Field Alignment with Dense Cores in the Transition between Cloud and Core Scales

In a magnetically dominated model of star formation, we expect to see alignments between the magnetic field orientation of star-forming dense cores and the cloud-scale magnetic field. A. Pandhi et al. showed instead, however, that the orientation of cores and their angular momentum vectors appear ra...

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מידע ביבליוגרפי

Principais autores:	Sean Yin, Ayush Pandhi, Rachel Friesen, Simon Coudé, Laura Fissel, Sarah Sadavoy, James Di Francesco, Doug Johnstone, Frédérick Poidevin, Mehrnoosh Tahani
פורמט:	Artigo
שפה:	Inglês
יצא לאור:	IOP Publishing 2026-01-01
סדרה:	The Astrophysical Journal
נושאים:	Submillimeter astronomy Star formation Interstellar medium Interstellar magnetic fields Polarimetry
גישה מקוונת:	https://doi.org/10.3847/1538-4357/ae6077
תגים:	הוספת תג אין תגיות, היה/י הראשונ/ה לתייג את הרשומה!