Takashi Shimonishi

CONCURRENT FORMATION OF CARBON AND SILICATE DUST IN NOVA V1280 SCO

We present infrared multi-epoch observations of the dust forming nova V1280 Sco over

SPECTRAL LINE SURVEY TOWARD A MOLECULAR CLOUD IN IC10

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THE DETECTION OF A HOT MOLECULAR CORE IN THE LARGE MAGELLANIC CLOUD WITH ALMA

2000 days from the outburst. The temporal evolution of the infrared spectral energy distributions at 1272, 1616 and 1947 days can be explained by the emissions produced by amorphous carbon dust of mass (6.6--8.7)

SPECTRAL LINE SURVEY TOWARD MOLECULAR CLOUDS IN THE LARGE MAGELLANIC CLOUD

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VLT/ISAAC infrared spectroscopy of embedded high-mass YSOs in the Large Magellanic Cloud: Methanol and the 3.47 μm band

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Adsorption Energies of Carbon, Nitrogen, and Oxygen Atoms on the Low-temperature Amorphous Water Ice: A Systematic Estimation from Quantum Chemistry Calculations

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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

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Carbon and silicate dust formation in V1280 Sco

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AKARI NIR spectroscopy of interstellar ices

with a representative grain size of 0.01

Near-Infrared Spectroscopy of Diffuse Galactic Radiation with AKARI/IRC

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