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Data supporting plots in Liu et al. 2026

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Zenodo2026-05-19 更新2026-05-26 收录
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https://zenodo.org/doi/10.5281/zenodo.18501394
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These are the parameters of the condensations identified in the ALMA dust continuum maps in the article "The dominance of turbulence over magnetism in the formation of massive star cluster seeds".  --------- region: source region. RA: in units of degrees. DEC: in units of degrees. major_FWHM: major FWHM of condensation in units of arcsec. minor_FWHM: minor FWHM of condensation in units of arcsec. PA_source: position angle of the condensation elongation orientation in units of degrees. PA_B: position angle of condensation-averaged magnetic field orientation in units of degrees. Ipeak_pbcor: peak intensity of condensation in units of Jy/beam. After primary beam correction. Fint_pbcor: integrated flux of condensation in units of Jy. After primary beam correction.
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2026-02-16
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