Showing 1–20 of 141 results
/ Date/ Name
Sep 21, 2010Aperture Synthesis Observations of CO, HCN, and 89GHz Continuum Emission toward NGC 604 in M 33: Sequential Star Formation Induced by Supergiant Hii regionJun 21, 2011NRO M33 All Disk Survey of Giant Molecular Clouds (NRO MAGiC): I. HI to H_2 TransitionMay 6, 2009Spatial correlation between submillimetre and Lyman-alpha galaxies in the SSA 22 protoclusterOct 3, 2023J0107a: A Barred Spiral Dusty Star-forming Galaxy at $z=2.467$Feb 4, 2013X-ray Detections of Sub-millimetre Galaxies: Active Galactic Nuclei Versus Starburst ContributionJun 5, 2018Expanding CO Shells in the Orion A Molecular CloudSep 12, 2019Nobeyama 45-m mapping observations toward nearby molecular clouds, Orion A, Aquila Rift, and M17: Project overviewApr 23, 2020Super-resolution Imaging of the Protoplanetary Disk HD 142527 Using Sparse ModelingJun 4, 2019Testing Star Formation Laws on Spatially Resolved Regions in a $z \approx 4.3$ Starburst GalaxyMar 18, 2019Nature of Faint Radio Sources in GOODS-North and GOODS-South Fields - I. Spectral Index and Radio-FIR CorrelationAug 6, 2018ALMA $^{12}$CO (J=1--0) imaging of the nearby galaxy M83: Variations in the efficiency of star formation in giant molecular cloudsMay 20, 2019Discovery of an au-scale excess in millimeter emission from the protoplanetary disk around TW HyaJun 27, 2019Nobeyama 45-m Mapping Observations toward Orion A. III. Multi-Line Observations toward an Outflow-shocked Region, OMC-2 FIRFeb 18, 1999NMA Survey of CO and HCN Emission from Nearby Active GalaxiesApr 27, 2007A Search for CO(J=3-2) Emission from the Host Galaxy of GRB 980425 with the Atacama Submillimeter Telescope ExperimentOct 27, 2014Phase Characteristics of the ALMA 3 km Baseline DataDec 31, 2016ALMA reveals Strong [CII] emission in a galaxy embedded in a giant Lyman-alpha blob at z=3.1Jan 11, 2017ALMA Long Baseline Campaigns: Phase Characteristics of Atmosphere at Long Baselines in the Millimeter and Submillimeter WavelengthsDec 13, 2016The 1.1 mm Continuum Survey of the Small Magellanic Cloud: Physical Properties and Evolution of the Dust-selected CloudsSep 10, 2013The Dynamical State of The Serpens South Filamentary Infrared Dark Cloud