• Beuther, H., Kuiper, R. & Tafalla, M. Star formation from low to high mass: a comparative view. Annu. Rev. Astron. Astrophys. 63, 1–44 (2025).

    Article 
    ADS 

    Google Scholar
     

  • Bonnell, I. A., Vine, S. G. & Bate, M. R. Massive star formation: nurture, not nature. Mon. Not. R. Astron. Soc. 349, 735–741 (2004).

    Article 
    ADS 

    Google Scholar
     

  • Zhang, Q. et al. Magnetic fields and massive star formation. Astrophys. J. 792, 116 (2014).

    Article 
    ADS 

    Google Scholar
     

  • Li, H.-B. et al. Self-similar fragmentation regulated by magnetic fields in a region forming massive stars. Nature 520, 518–521 (2015).

    Article 
    ADS 

    Google Scholar
     

  • Planck Collaboration et al. Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds. Astron. Astrophys. 586, A138 (2016).

    Article 

    Google Scholar
     

  • Kauffmann, J., Pillai, T. & Goldsmith, P. F. Low virial parameters in molecular clouds: implications for high-mass star formation and magnetic fields. Astrophys. J. 779, 185 (2013).

    Article 
    ADS 

    Google Scholar
     

  • Liu, J., Qiu, K. & Zhang, Q. Magnetic Fields in star formation: a complete compilation of all the DCF estimations. Astrophys. J. 925, 30 (2022).

    Article 
    ADS 

    Google Scholar
     

  • Mouschovias, T. C. Nonhomologous contraction and equilibria of self-gravitating, magnetic interstellar clouds embedded in an intercloud medium: star formation. II. Results. Astrophys. J. 207, 141–158 (1976).

    Article 
    ADS 

    Google Scholar
     

  • Nakamura, F. & Li, Z.-Y. Magnetically regulated star formation in three dimensions: the case of the Taurus molecular cloud complex. Astrophys. J. 687, 354–375 (2008).

    Article 
    ADS 

    Google Scholar
     

  • Tassis, K., Dowell, C. D., Hildebrand, R. H., Kirby, L. & Vaillancourt, J. E. Statistical assessment of shapes and magnetic field orientations in molecular clouds through polarization observations. Mon. Not. R. Astron. Soc. 399, 1681–1693 (2009).

    Article 
    ADS 

    Google Scholar
     

  • Beltrán, M. T. et al. Self-similarity of the magnetic field at different scales: the case of G31.41+0.31. Astron. Astrophys. 686, A281 (2024).

    Article 

    Google Scholar
     

  • Lebreuilly, U. et al. The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps. Astron. Astrophys. 701, A217 (2025).

    Article 

    Google Scholar
     

  • Beuther, H. et al. Gravity and rotation drag the magnetic field in high-mass star formation. Astrophys. J. 904, 168 (2020).

    Article 
    ADS 

    Google Scholar
     

  • Klos, K. S., Bonnell, I. A. & Smith, R. J. The role of magnetic fields in the formation of high-mass star-forming cores. Mon. Not. R. Astron. Soc. 539, 2307–2322 (2025).

    Article 
    ADS 

    Google Scholar
     

  • Li, H.-b., Fang, M., Henning, T. & Kainulainen, J. The link between magnetic fields and filamentary clouds: bimodal cloud orientations in the Gould belt. Mon. Not. R. Astron. Soc. 436, 3707–3719 (2013).

    Article 
    ADS 

    Google Scholar
     

  • Sanhueza, P. et al. Gravity-driven magnetic field at 1000 au scales in high-mass star formation. Astrophys. J. Lett. 915, L10 (2021).

    Article 
    ADS 

    Google Scholar
     

  • Cortés, P. C. et al. Magnetic Fields in Massive Star-forming Regions (MagMaR). II. Tomography through dust and molecular line polarization in NGC 6334I(N). Astrophys. J. 923, 204 (2021).

    Article 
    ADS 

    Google Scholar
     

  • Fernández-López, M. et al. Magnetic Fields in Massive Star-forming Regions (MagMaR). I. Linear polarized imaging of the ultracompact H II region G5.89-0.39. Astrophys. J. 913, 29 (2021).

    Article 
    ADS 

    Google Scholar
     

  • Cortés, P. C. et al. MagMaR III—resisting the pressure, is the magnetic field overwhelmed in NGC6334I? Astrophys. J. 972, 115 (2024).

    Article 
    ADS 

    Google Scholar
     

  • Saha, P. et al. Magnetic Fields in Massive Star-forming Regions (MagMaR): unveiling an hourglass magnetic field in G333.46–0.16 using ALMA. Astrophys. J. Lett. 972, L6 (2024).

    Article 
    ADS 

    Google Scholar
     

  • Zapata, L. A. et al. Magnetic Fields in Massive Star-forming Regions (MagMaR). IV. Tracing the magnetic fields in the O-type protostellar system IRAS 16547–4247. Astrophys. J. 974, 257 (2024).

    Article 
    ADS 

    Google Scholar
     

  • Sanhueza, P. et al. Magnetic Fields in Massive Star-forming Regions (MagMaR). V. The magnetic field at the onset of high-mass star formation. Astrophys. J. 980, 87 (2025).

    Article 
    ADS 

    Google Scholar
     

  • Rosolowsky, E. W., Pineda, J. E., Kauffmann, J. & Goodman, A. A. Structural analysis of molecular clouds: dendrograms. Astrophys. J. 679, 1338–1351 (2008).

    Article 
    ADS 

    Google Scholar
     

  • Men’shchikov, A. Multiscale, multiwavelength extraction of sources and filaments using separation of the structural components: getsf. Astron. Astrophys. 649, A89 (2021).

    Article 
    ADS 

    Google Scholar
     

  • Padoan, P. et al. Theoretical models of polarized dust emission from protostellar cores. Astrophys. J. 559, 1005–1018 (2001).

    Article 
    ADS 

    Google Scholar
     

  • Soler, J. D. et al. The relation between the column density structures and the magnetic field orientation in the Vela C molecular complex. Astron. Astrophys. 603, A64 (2017).

    Article 

    Google Scholar
     

  • Misugi, Y., Inutsuka, S.-i. & Arzoumanian, D. Evolution of the angular momentum of molecular cloud cores formed from filament fragmentation. Astrophys. J. 943, 76 (2023).

    Article 
    ADS 

    Google Scholar
     

  • Ishihara, K. et al. Digging into the Interior of Hot Cores with ALMA (DIHCA). IV. Fragmentation in high-mass star-forming clumps. Astrophys. J. 974, 95 (2024).

    Article 
    ADS 

    Google Scholar
     

  • Motte, F. et al. ALMA-IMF. I. Investigating the origin of stellar masses: Introduction to the large program and first results. Astron. Astrophys. 662, A8 (2022).

    Article 

    Google Scholar
     

  • Tan, J. C. et al. in Protostars and Planets VI (eds Beuther, H. et al.) 149–172 (Univ. Arizona Press, 2014).

  • Commerçon, B., Hennebelle, P. & Henning, T. Collapse of massive magnetized dense cores using radiation magnetohydrodynamics: early fragmentation inhibition. Astrophys. J. Lett. 742, L9 (2011).

    Article 
    ADS 

    Google Scholar
     

  • Palau, A. et al. Does the magnetic field suppress fragmentation in massive dense cores? Astrophys. J. 912, 159 (2021).

    Article 
    ADS 

    Google Scholar
     

  • Beuther, H. et al. Density distributions, magnetic field structures, and fragmentation in high-mass star formation. Astron. Astrophys. 682, A81 (2024).

    Article 

    Google Scholar
     

  • Liu, J. et al. Magnetic fields in the early stages of massive star formation as revealed by ALMA. Astrophys. J. 895, 142 (2020).

    Article 
    ADS 

    Google Scholar
     

  • Liu, J. et al. Multi-scale physical properties of NGC 6334 as revealed by local relative orientations between magnetic fields, density gradients, velocity gradients, and gravity. Astrophys. J. 945, 160 (2023).

    Article 
    ADS 

    Google Scholar
     

  • Liu, J. et al. Dark dragon breaks magnetic chain: dynamical substructures of IRDC G28.34 form in supported environments. Astrophys. J. 966, 120 (2024).

    Article 
    ADS 

    Google Scholar
     

  • Zhang, Y., Guo, Z., Wang, H. H. & Li, H. B. Anchoring magnetic fields in turbulent molecular clouds. II. From 0.1 to 0.01 pc. Astrophys. J. 871, 98 (2019).

    Article 
    ADS 

    Google Scholar
     

  • Allen, A., Li, Z.-Y. & Shu, F. H. Collapse of magnetized singular isothermal toroids. II. Rotation and magnetic braking. Astrophys. J. 599, 363–379 (2003).

    Article 
    ADS 

    Google Scholar
     

  • Wurster, J. & Li, Z.-Y. The role of magnetic fields in the formation of protostellar discs. Front. Astron. Space Sci. 5, 39 (2018).

    Article 
    ADS 

    Google Scholar
     

  • Frank, A. et al. in Protostars and Planets VI (eds Beuther, H. et al.) 451–474 (Univ. Arizona Press, 2014).

  • Ohashi, N., Hayashi, M., Ho, P. T. P. & Momose, M. Interferometric imaging of IRAS 04368+2557 in the L1527 molecular cloud core: a dynamically infalling envelope with rotation. Astrophys. J. 475, 211–223 (1997).

    Article 
    ADS 

    Google Scholar
     

  • Mininni, C. et al. ALMAGAL. IV. Morphological comparison of molecular and thermal dust emission using the histogram of oriented gradients method. Astron. Astrophys. 699, A34 (2025).

    Article 

    Google Scholar
     

  • Machida, M. N., Matsumoto, T., Hanawa, T. & Tomisaka, K. Evolution of rotating molecular cloud core with oblique magnetic field. Astrophys. J. 645, 1227–1245 (2006).

    Article 
    ADS 

    Google Scholar
     

  • Joos, M., Hennebelle, P., Ciardi, A. & Fromang, S. The influence of turbulence during magnetized core collapse and its consequences on low-mass star formation. Astron. Astrophys. 554, A17 (2013).

    Article 
    ADS 

    Google Scholar
     

  • Lazarian, A. Tracing magnetic fields with aligned grains. J. Quant. Spectrosc. Radiat. Transf. 106, 225–256 (2007).

    Article 
    ADS 

    Google Scholar
     

  • McMullin, J. P., Waters, B., Schiebel, D., Young, W. & Golap, K. in Astronomical Data Analysis Software and Systems XVI, Vol. 376 (eds Shaw, R. A. et al.) 127–130 (ASP, 2007).

  • Olguin, F. A. et al. Digging into the Interior of Hot Cores with ALMA (DIHCA). I. Dissecting the high-mass star-forming core G335.579-0.292 MM1. Astrophys. J. 909, 199 (2021).

    Article 
    ADS 

    Google Scholar
     

  • Vaillancourt, J. E. Placing confidence limits on polarization measurements. Publ. Astron. Soc. Pac. 118, 1340–1343 (2006).

    Article 
    ADS 

    Google Scholar
     

  • Naghizadeh-Khouei, J. & Clarke, D. On the statistical behaviour of the position angle of linear polarization. Astron. Astrophys. 274, 968 (1993).

    ADS 

    Google Scholar
     

  • Girart, J. M. et al. Resolving the polarized dust emission of the disk around the massive star powering the HH 80-81 radio jet. Astrophys. J. Lett. 856, L27 (2018).

    Article 
    ADS 

    Google Scholar
     

  • Contreras, Y. et al. Infall signatures in a prestellar core embedded in the high-mass 70 μm dark IRDC G331.372-00.116. Astrophys. J. 861, 14 (2018).

    Article 
    ADS 

    Google Scholar
     

  • Liu, J. et al. Calibrating the Davis–Chandrasekhar–Fermi method with numerical simulations: uncertainties in estimating the magnetic field strength from statistics of field orientations. Astrophys. J. 919, 79 (2021).

    Article 
    ADS 

    Google Scholar
     

  • Teyssier, R. Cosmological hydrodynamics with adaptive mesh refinement. A new high resolution code called RAMSES. Astron. Astrophys. 385, 337–364 (2002).

    Article 
    ADS 

    Google Scholar
     

  • Mouschovias, T. C. & Spitzer, J. L. Note on the collapse of magnetic interstellar clouds. Astrophys. J. 210, 326 (1976).

    Article 
    ADS 

    Google Scholar
     

  • Hennebelle, P. et al. Collapse, outflows and fragmentation of massive, turbulent and magnetized prestellar barotropic cores. Astron. Astrophys. 528, A72 (2011).

    Article 

    Google Scholar
     

  • Truelove, J. K. et al. The Jeans condition: a new constraint on spatial resolution in simulations of isothermal self-gravitational hydrodynamics. Astrophys. J. Lett. 489, L179–L183 (1997).

    Article 
    ADS 

    Google Scholar
     

  • Bleuler, A. & Teyssier, R. Towards a more realistic sink particle algorithm for the RAMSES code. Mon. Not. R. Astron. Soc. 445, 4015–4036 (2014).

    Article 
    ADS 

    Google Scholar
     

  • Reissl, S., Wolf, S. & Brauer, R. Radiative transfer with POLARIS. I. Analysis of magnetic fields through synthetic dust continuum polarization measurements. Astron. Astrophys. 593, A87 (2016).

    Article 
    ADS 

    Google Scholar
     

  • Houde, M., Hull, C. L. H., Plambeck, R. L., Vaillancourt, J. E. & Hildebrand, R. H. Dispersion of magnetic fields in molecular clouds. IV. Analysis of interferometry data. Astrophys. J. 820, 38 (2016).

    Article 
    ADS 

    Google Scholar
     

  • Taniguchi, K. et al. Digging into the Interior of Hot Cores with the ALMA (DIHCA). III. The chemical link between NH2CHO, HNCO, and H2CO. Astrophys. J. 950, 57 (2023).

    Article 
    ADS 

    Google Scholar
     

  • Schöier, F. L., van der Tak, F. F. S., van Dishoeck, E. F. & Black, J. H. An atomic and molecular database for analysis of submillimetre line observations. Astron. Astrophys. 432, 369–379 (2005).

    Article 
    ADS 

    Google Scholar
     

  • Goodman, A. A., Benson, P. J., Fuller, G. A. & Myers, P. C. Dense cores in dark clouds. VIII. Velocity gradients. Astrophys. J. 406, 528 (1993).

    Article 
    ADS 

    Google Scholar
     

  • Liu, J. Data supporting Liu et al. 2026. Zenodo https://doi.org/10.5281/zenodo.19062258 (2026).

  • Astropy Collaboration et al. Astropy: a community Python package for astronomy. Astron. Astrophys. 558, A33 (2013).

    Article 

    Google Scholar
     

  • Hunter, J. D. Matplotlib: a 2D graphics environment. Comput. Sci. Eng. 9, 90–95 (2007).

    Article 

    Google Scholar