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Recent progress in theory and observational study of dust grain alignment and rotational disruption in star-forming regions
Modern understanding of dust astrophysics reveals that radiative torques (RATs) arising
from the radiation–dust interaction can induce two fundamental effects: grain alignment and …
from the radiation–dust interaction can induce two fundamental effects: grain alignment and …
Submillimeter and far-infrared polarimetric observations of magnetic fields in star-forming regions
K Pattle, L Fissel - Frontiers in Astronomy and Space Sciences, 2019 - frontiersin.org
Observations of star-forming regions by the current and upcoming generation of
submillimeter polarimeters will shed new light on the evolution of magnetic fields over the …
submillimeter polarimeters will shed new light on the evolution of magnetic fields over the …
Magnetic fields in star formation: from clouds to cores
K Pattle, L Fissel, M Tahani, T Liu… - ar** analysis computations
ABD Nandiyanto… - ASEAN …, 2023 - ejournal.bumipublikasinusantara.id
This study examines the map** of research bibliometric data analysis related to resin-
based brake pads. The research data was collected through the publish or perish reference …
based brake pads. The research data was collected through the publish or perish reference …
Magnetized filamentary gas flows feeding the young embedded cluster in Serpens South
Observations indicate that molecular clouds are strongly magnetized, and that magnetic
fields influence the formation of stars. A key observation supporting the conclusion that …
fields influence the formation of stars. A key observation supporting the conclusion that …
HAWC+/SOFIA multiwavelength polarimetric observations of OMC-1
We report new polarimetric and photometric maps of the massive star-forming region OMC-1
using the HAWC+ instrument on the Stratospheric Observatory for Infrared Astronomy. We …
using the HAWC+ instrument on the Stratospheric Observatory for Infrared Astronomy. We …
Magnetic fields in star formation: a complete compilation of all the DCF estimations
J Liu, K Qiu, Q Zhang - The Astrophysical Journal, 2022 - iopscience.iop.org
Abstract The Davis–Chandrasekhar–Fermi (DCF) method provides an indirect way to
estimate the magnetic field strength from statistics of magnetic field orientations. We compile …
estimate the magnetic field strength from statistics of magnetic field orientations. We compile …
The Rate, Amplitude, and Duration of Outbursts from Class 0 Protostars in Orion
W Zakri, ST Megeath, WJ Fischer… - The Astrophysical …, 2022 - iopscience.iop.org
At least half of a protostar's mass is accreted in the Class 0 phase, when the central protostar
is deeply embedded in a dense, infalling envelope. We present the first systematic search …
is deeply embedded in a dense, infalling envelope. We present the first systematic search …