Showing 1–20 of 35 results
/ Date/ Name
Feb 22, 2021Gas infalling motions in the envelopes of Very Low Luminosity ObjectsOct 14, 2025YSO Variability in the W51 Star-Forming RegionJun 15, 2021Mid-$J$ CO Line Observations of Protostellar Outflows in the Orion Molecular CloudsMar 3, 2021Revealing the diverse magnetic field morphologies in Taurus dense cores with sensitive sub-millimeter polarimetryDec 8, 2020Observations of magnetic fields surrounding LkH$α$ 101 taken by the BISTRO survey with JCMT-POL-2Dec 19, 2018CO Outflow Survey of 68 Very Low Luminosity Objects: a Search for Proto-Brown Dwarf CandidatesSep 7, 2017How do stars gain their mass? A JCMT/SCUBA-2 Transient Survey of Protostars in Nearby Star Forming RegionsFeb 20, 2019The JCMT BISTRO Survey: The Magnetic Field In The Starless Core $ρ$ Ophiuchus CJul 1, 2020The JCMT BISTRO Survey: Magnetic Fields Associated with a Network of Filaments in NGC 1333Dec 10, 2008The Spitzer c2d Survey of Nearby Dense Cores. V. Discovery of a VeLLO in the "Starless" Dense Core L328Jan 23, 2024Filamentary Network and Magnetic Field Structures Revealed with BISTRO in the High-Mass Star-Forming Region NGC2264 : Global Properties and Local Magnetogravitational ConfigurationsApr 25, 2018A First Look at BISTRO Observations of The $ρ$ Oph-A coreDec 21, 2022JCMT BISTRO Observations: Magnetic Field Morphology of Bubbles Associated with NGC 6334Jan 7, 2024The JCMT Transient Survey: Six-Year Summary of 450/850\,$μ$m Protostellar Variability and Calibration Pipeline Version 2.0Sep 28, 2021The JCMT BISTRO Survey: An 850/450$μ$m Polarization Study of NGC 2071IR in OrionBMay 16, 2018Magnetic fields towards Ophiuchus-B derived from SCUBA-2 polarization measurementsMay 23, 2016Dense Molecular Cores Being Externally HeatedNov 4, 2024The JCMT BISTRO Survey: The Magnetic Fields of the IC 348 Star-forming RegionFeb 23, 2023First BISTRO observations of the dark cloud Taurus L1495A-B10: the role of the magnetic field in the earliest stages of low-mass star formationNov 26, 2025Refined classification of YSOs and AGB stars by IR magnitudes, colors, and time-domain analysis with machine learning