141 citations · 314 across the 8 of their papers we have counts for
8 papers
Mid-infrared spectra of the shocked Murchison CM chondrite: Comparison with astronomical observations of dust in debris disks
A. Morlok, C. Koike, N. Tomioka +2
We present laboratory mid-infrared transmission/absorption spectra obtained from matrix of the hydrated Murchison CM meteorite experimentally shocked at peak pressures of 10 to 49…
Mid-infrared spectra of differentiated meteorites (achondrites): Comparison with astronomical observations of dust in protoplanetary and debris disks
A. Morlok, C. Koike, K. Tomeoka +4
Mid-infrared (5 micron to 25 micron) transmission/absorption spectra of differentiated meteorites (achondrites) were measured to permit comparison with astronomical observations of…
Radiative equilibrium estimates of dust temperature and mass in high-redshift galaxies
Akio K. Inoue, Takuya Hashimoto, Hiroki Chihara +1
Estimating the temperature and mass of dust in high- galaxies is essential for discussions of the origin of dust in the early Universe. However, this suffers from limited sampli…
Morphological effects on IR band profiles: Experimental spectroscopic analysis with application to observed spectra of oxygen-rich AGB stars
A. Tamanai, H. Mutschke, J. Blum +3
To trace the source of the unique 13, 19.5, and 28 m emission features in the spectra of oxygen-rich circumstellar shells around AGB stars, we have compared dust extinction spec…
Photo-Luminescence and Possible Forsterite nanoparticles Model of Extended Red Emission
K. Koike, H. Chihara, C. Koike +4
Possible forsterite nanoparticle model of the Extended Red Emission(ERE) is proposed on the basis of photo-luminescence of forsterite after gamma-ray and neutron irradiation. Forst…
PAHs and crystalline silicates in the post-AGB star IRAS 16279-4757
M. Matsuura, A. A. Zijlstra, F. J. Molster +7
IRAS 16279-4757 belongs to a group of post-AGB stars showing both PAH bands and crystalline silicates. We present mid-infrared images, that resolve the object for the first time. T…