Kei Fukue

New Panoramic View of 12CO and 1.1 mm Continuum Emission in the Orion A Giant Molecular Cloud. I. Survey Overview and Possible External Triggers of Star Formation

We present new, wide and deep images in the 1.1 mm continuum and the

KINEMATICS OF CLASSICAL CEPHEIDS IN THE NUCLEAR STELLAR DISK

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High sensitivity, wide coverage, and high-resolution NIR non-cryogenic spectrograph, WINERED

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ZnSe immersion grating in the short NIR region

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Correction of Near-infrared High-resolution Spectra for Telluric Absorption at 0.90–1.35 μm

=1-0) emission toward the northern part of the Orion A Giant Molecular Cloud (Orion-A GMC). The 1.1 mm data were taken with the AzTEC camera mounted on the Atacama Submillimeter Telescope Experiment (ASTE) 10 m telescope in Chile, and the

Method to estimate the effective temperatures of late-type giants using line-depth ratios in the wavelength range 0.97–1.32 μm

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New Classical Cepheids in the Inner Part of the Northern Galactic Disk, and Their Kinematics

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LINE-DEPTH RATIOS IN H-BAND SPECTRA TO DETERMINE EFFECTIVE TEMPERATURES OF G- AND K-TYPE GIANTS AND SUPERGIANTS

J

On the Chemical Abundances of Miras in Clusters: V1 in the Metal-rich Globular NGC 5927

=1-0) data were with the 25 beam receiver (BEARS) on the NRO 45 m telescope in the On-The-Fly (OTF) mode. The present AzTEC observations are the widest

Optical and Near-infrared High-resolution Spectroscopic Observations of Nova V2659 Cyg: Structure of Nova Ejecta and Origin of Two-distinct Velocity Systems

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