Showing 1–20 of 24 results
/ Date/ Name
Apr 13, 2026JWST Observations of Starbursts: Dust Processing in the M82 SuperwindJul 15, 2025The ALMA-CRISTAL survey: Resolved kinematic studies of main sequence star-forming galaxies at 4<z<6Dec 23, 2024A Tale of Three: Magnetic Fields along the Orion Integral-Shaped Filament as Revealed by JCMT BISTRO surveyNov 4, 2024The JCMT BISTRO Survey: The Magnetic Fields of the IC 348 Star-forming RegionOct 11, 2024JWST/MIRI Observations of Newly Formed Dust in the Cold, Dense Shell of the Type IIn SN 2005ipMay 9, 2024REBELS-25: Discovery of a dynamically cold disc galaxy at z = 7.31Sep 22, 2023JWST NIRCam Observations of SN 1987A: Spitzer Comparison and Spectral DecompositionMay 18, 2023The JCMT BISTRO Survey: Studying the Complex Magnetic Field of L43Feb 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 formationJan 25, 2023JWST Discovery of Dust Reservoirs in Nearby Type IIP Supernovae 2004et and 2017eawDec 21, 2022JCMT BISTRO Observations: Magnetic Field Morphology of Bubbles Associated with NGC 6334Dec 5, 2022The JCMT BISTRO-2 Survey: Magnetic Fields of the Massive DR21 FilamentOct 12, 2022The JCMT BISTRO Survey: A Spiral Magnetic Field in a Hub-filament Structure, Monoceros R2Aug 17, 2022The ALMA REBELS Survey: The Dust-obscured Cosmic Star Formation Rate Density at Redshift 7Apr 29, 2022Dust masses for a large sample of core-collapse supernovae from optical emission line asymmetries: dust formation on 30-year timescalesMar 28, 2022The ALMA REBELS Survey: Dust Continuum Detections at z > 6.5Jan 13, 2022B-fields in Star-Forming Region Observations (BISTRO): Magnetic Fields in the Filamentary Structures of Serpens MainSep 28, 2021The JCMT BISTRO Survey: An 850/450$μ$m Polarization Study of NGC 2071IR in OrionBMar 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-2