Where stars form

Magnetic fields, cores and gas flows inside individual molecular clouds: Orion, Monoceros OB1, infrared dark clouds and the centre of NGC 253.

30′ · 6.5 pc
SHASSA Hα 48″
ALMA · JCMT · JWST · TRAO

Inside a single cloud the field is measured with submillimetre polarimeters such as POL-2 on the JCMT and with ALMA, and compared with the gas motions traced by molecular lines. The question in each case is the same: does the field guide the gas into cores, or do gravity and turbulence win?

Results

What the papers report, in their own terms. Each item links to its source.

  1. In Monoceros OB1 East the large-scale field is ordered. In the northern part it runs mostly along the filaments; the southern part has at least two regions with distinct field orientations.

    Alina et al. 2022
  2. In the translucent high-latitude cloud MBM 12, column density structures change from parallel to perpendicular to the Planck field above a threshold column density.

    N(H2) = 4.5 × 1021 cm-2

    Vorster et al. 2026
  3. In the infrared dark cloud G34.43+0.24, JCMT POL-2 shows an ordered field close to perpendicular to the filament around its central clumps. The cloud is marginally critical, with mass-to-flux ratios near one in all three parts.

    BPOS = 470 ± 190, 100 ± 40, 60 ± 34 µG (centre, north, south)

    Soam et al. 2019
  4. JWST and ALMA show a compact hub-filament system in the protocluster G286.21+0.17, about 0.5 pc across, with at least four filaments converging on a dense hub. The filament accretion rates and the radial distribution of cores are consistent with competitive accretion.

    filament accretion rates 7.6–11 × 10-5 M☉ yr-1

    Dewangan et al. 2026

Monoceros OB1 East

The Planck field over the cloud and the regions where Alina et al. 2022 measured its strength and traced the gas motions.

Multi-band image of Monoceros OB1 East: Herschel 250 µm dust in red, WISE 12 µm in teal, H-alpha in blueNMNWNEShockABNENGC 2264
7′ beam5 pc
Galactic coordinates, b up and l increasing to the left, 3° wide around l = 202.9°, b = 1.9°; the compass shows equatorial north and east, which the paper's region names follow. White segments: plane-of-sky field from Planck PR4 353 GHz, smoothed to 7′ as in the paper and drawn one per beam where the angle uncertainty is below 10°, one of the paper's two cuts (it also required a polarization signal to noise of at least 2). Outlines are traced from the paper's figures to about 1′: white, the velocity-coherent structures of the northern filaments (Fig. 6); red, the candidate shock between them (Fig. 9b); grey, rectangles A and B in the south (Fig. 12). The paper used Planck PR3; these segments are recomputed here.

Papers

19 entries from NASA ADS. All publications →

  1. 2026
    Discovery of a compact hub-filament system in G286.21 + 0.17 with JWST and ALMA: insights into protocluster formation and competitive accretionDewangan, Bhadari, Yadav, … Alina (9 of 20) et al.Monthly Notices of the Royal Astronomical Society, 552, stag1764 · arXiv:2605.14693
  2. 2026
  3. 2026
  4. 2026
    MAJORS II: HCO+ and HCN abundances in W40Plume, Eden, Currie, … Alina (18 of 37) et al.Monthly Notices of the Royal Astronomical Society, 547, stag186 · arXiv:2601.19971
  5. 2025
    Magnetic Field of a Ring-like Molecular CloudAlina, Umirbayeva, Doi et al.The Astronomical Journal, 170, 152 · arXiv:2507.19281
  6. 2025
    The dust polarisation and magnetic field structure in the centre of NGC253 with ALMABelfiori, Paladino, Hughes, … Alina (5 of 10) et al.Astronomy and Astrophysics, 697, A24 · arXiv:2503.03493
    4 cit.
  7. 2025
  8. 2024
    The Magnetic Field in Quiescent Star-forming Filament G16.96+0.27Gu, Liu, Shen, … Alina (22 of 23) et al.The Astrophysical Journal, 976, 249 · arXiv:2410.15913
    6 cit.
  9. 2024
    On the Scarcity of Dense Cores (n > 105 cm−3) in High-latitude Planck Galactic Cold ClumpsXu, Wang, Liu, … Alina (24 of 37) et al.The Astrophysical Journal Letters, 963, L9 · arXiv:2401.14658
    3 cit.
  10. 2022
    Large-scale magnetic field in the Monoceros OB 1 east molecular cloudAlina, Montillaud, Hu et al.Astronomy and Astrophysics, 658, A90 · arXiv:2007.15344
    26 cit.
  11. 202132 cit.
  12. 2019
    Multi-scale analysis of the Monoceros OB 1 star-forming region. II. Colliding filaments in the Monoceros OB1 molecular cloudMontillaud, Juvela, Vastel, … Alina (17 of 27) et al.Astronomy and Astrophysics, 631, A3 · arXiv:1909.06145
    29 cit.
  13. 2019
    Multi-scale analysis of the Monoceros OB 1 star-forming region. I. The dense core populationMontillaud, Juvela, Vastel, … Alina (17 of 27) et al.Astronomy and Astrophysics, 631, L1 · arXiv:1909.03781
    12 cit.
  14. 2019
    Magnetic Fields in the Infrared Dark Cloud G34.43+0.24Soam, Liu, Andersson, … Alina (34 of 43) et al.The Astrophysical Journal, 883, 95 · arXiv:1908.03624
    55 cit.
  15. 2019
    SCOPE: SCUBA-2 Continuum Observations of Pre-protostellar Evolution - survey description and compact source catalogueEden, Liu, Kim, … Alina (62 of 163) et al.Monthly Notices of the Royal Astronomical Society, 485, 2895 · arXiv:1902.10180
    43 cit.
  16. 2018
    Dust spectrum and polarisation at 850 μm in the massive IRDC G035.39-00.33Juvela, Guillet, Liu, … Alina (6 of 21) et al.Astronomy and Astrophysics, 620, A26 · arXiv:1809.00864
    27 cit.
  17. 2018
    A Holistic Perspective on the Dynamics of G035.39-00.33: The Interplay between Gas and Magnetic FieldsLiu, Li, Juvela, … Alina (37 of 57) et al.The Astrophysical Journal, 859, 151 · arXiv:1803.09457
    81 cit.
  18. 2018
    The TOP-SCOPE Survey of PGCCs: PMO and SCUBA-2 Observations of 64 PGCCs in the Second Galactic QuadrantZhang, Liu, Yuan, … Alina (22 of 26) et al.The Astrophysical Journal Supplement Series, 236, 49 · arXiv:1805.03883
    15 cit.
  19. 2018
    The TOP-SCOPE Survey of Planck Galactic Cold Clumps: Survey Overview and Results of an Exemplar Source, PGCC G26.53+0.17Liu, Kim, Juvela, … Alina (51 of 156) et al.The Astrophysical Journal Supplement Series, 234, 28 · arXiv:1711.04382
    65 cit.