Yuri Nishimura
0000-0003-0563-067X
Institute of Astronomy, The University of Tokyo
11 papers found
Refreshing results…
Chemistry and Physics of a Low-metallicity Hot Core in the Large Magellanic Cloud
Molecular Gas Density Measured with H2CO and CS toward a Spiral Arm of M51
A 3 mm Spectral Line Survey toward the Barred Spiral Galaxy NGC 3627
The Excitation State of Galactic Diffuse Molecular Gas, Investigated with ALMA Observations of Multi-transition Absorption Lines
Molecular-cloud-scale Chemical Composition. III. Constraints of Average Physical Properties through Chemical Models
A Multiline Study of a High-mass Young Stellar Object in the Small Magellanic Cloud with ALMA: The Detection of Methanol Gas at 0.2 Solar Metallicity
Diverse Nuclear Star-forming Activities in the Heart of NGC 253 Resolved with 10-pc-scale ALMA Images
Molecular-cloud-scale Chemical Composition. II. Mapping Spectral Line Survey toward W3(OH) in the 3 mm Band
Molecular-cloud-scale Chemical Composition. I. A Mapping Spectral Line Survey toward W51 in the 3 mm Band
Spectral Line Survey Toward a Molecular Cloud in Ic10
Spectral Line Survey Toward Molecular Clouds in the Large Magellanic Cloud
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