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- W4384268503 abstract "This paper presents the results of full polarization observations of the massive star-forming region W75N, conducted with 3 arcsec spatial resolutions at 345 GHz using the Submillimeter Array (SMA). The magnetic field structures in the dense cores of the region are derived using the linearly polarized continuum emission. The overall magnetic field strength and orientation are found to agree with those from the previous observations. The plane-of-sky (POS) component of the magnetic field in the region was calculated to be 0.8 pm 0.1 mG using the angular dispersion function (ADF) method. Further analyses involving the polarization-intensity gradient-local gravity method and H13CO+ (4-3) line data indicated that the cloud is undergoing global gravitational collapse and the magnetic field is shaped by gravity and outflows in the dense core regions." @default.
- W4384268503 created "2023-07-14" @default.
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- W4384268503 date "2023-07-12" @default.
- W4384268503 modified "2023-10-17" @default.
- W4384268503 title "Submillimeter Observations of Magnetic Fields in Massive Star-forming Region W75N" @default.
- W4384268503 doi "https://doi.org/10.48550/arxiv.2307.06231" @default.
- W4384268503 hasPublicationYear "2023" @default.
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