Showing 1–20 of 32 results
/ Date/ Name
Jan 11, 2011Planck Early Results: The submillimetre properties of a sample of Galactic cold clumpsFeb 4, 2022Chemical exploration of Galactic cold coresJun 17, 2022ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- XI. From inflow to infall in hub-filament systemsJul 22, 2014Dust properties inside molecular clouds from coreshine modeling and observationsDec 16, 2020ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Detection of extremely high density compact structure of prestellar cores and multiple substructures withinJan 10, 2024The magnetic field in colliding filaments G202.3+2.5Sep 4, 2018Dust spectrum and polarisation at 850 um in the massive IRDC G035.39-00.33Oct 23, 2018Dust polarisation studies on MHD simulations of molecular clouds: methods comparison for the relative orientations analysisSep 13, 2019Multi-scale analysis of the Monoceros OB 1 star-forming region: II. Colliding filaments in the Monoceros OB1 molecular cloudMay 8, 2021ATOMS:ALMA Three-millimeter Observations of Massive Star-forming regions -- III :Catalogues of candidate hot molecular cores and Hyper/Ultra compact HII regionsOct 21, 2024The magnetic field in quiescent star-forming filament G16.96+0.27Sep 9, 2019Multi-scale analysis of the Monoceros OB 1 star-forming region: I. The dense core populationDec 7, 2009L1506: a prestellar core in the makingFeb 14, 2023Density Structure of Centrally Concentrated Prestellar Cores from Multi-scale ObservationsJun 17, 2023Direct observational evidence of the multi-scale, dynamical mass accretion toward a high-mass star forming hub-filament systemJan 26, 2024On the Scarcity of Dense Cores ($n>10^{5}$ cm$^{-3}$) in High Latitude Planck Galactic Cold ClumpsJul 19, 2019Galactic continuum surveys with the new 850 micron MKID camera at the EAO/JCMT 15-m telescopeAug 9, 2019Synthetic observations of dust emission and polarisation of Galactic cold clumpsMay 29, 2016Star formation laws in both Galactic massive clumps and external galaxies: An extensive study with dust continuum, HCN (4-3), and CS (7-6)Dec 1, 2016Astrochemical Properties of Planck Cold Clumps