9 datasets found

Keywords: molecular clouds

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  • WISDOM Project IX study of GMCs in NGC 4429

    We present high spatial resolution (~= 12 pc) Atacama Large Millimeter/submillimeter Array 12CO(J = 3-2) observations of the nearby lenticular galaxy NGC 4429. We identify 217...
  • ATOMS Paper III, massive star-forming regions

    We have identified 453 compact dense cores in 3 mm continuum emission maps in the ALMA Three-millimetre Observations of Massive Star-forming regions survey, and compiled three...
  • GMC's properties cat. in Cen A mol. disc

    We present the first census of giant molecular clouds (GMCs) complete down to 106 M_{sun} and within the inner 4 kpc of the nearest giant elliptical and powerful radio galaxy,...
  • Fractionation in young cores

    Nitrogen fractionation is a powerful tracer of the chemical evolution during star- and planet formation. This requires robust determinations of the nitrogen fractionation across...
  • A Galactic survey of radio jets from MYSOs

    In conjunction with a previous southern-hemisphere work, we present the largest radio survey of jets from massive protostars to date with high-resolution (~0.04 arcsec) Jansky...
  • Mon OB4 a new association in Gaia DR2

    We use Gaia DR2 data to survey the classic Monoceros OB1 region and look for the existence of a dispersed young population, co-moving with the cloud complex. An analysis of the...
  • ALMA-IRDC from cloud to core scales

    Infrared dark clouds (IRDCs) are potential hosts of the elusive early phases of high mass star formation (HMSF). Here, we conduct an in-depth analysis of the fragmentation...
  • Magnetic field in the Flame nebula

    Star formation is essential in galaxy evolution and the cycling of matter. The support of interstellar clouds against gravitational collapse by magnetic (B-) fields has been...
  • NH3 Observations of Cygnus X

    The physical properties, evolution, and fragmentation of massive dense cores (MDCs, ~0.1pc) are fundamental to the understanding of high-mass star formation. We aim at...
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