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( Hidehiro Okada ) 한국알타이학회 2005 알타이학보 Vol.0 No.15
Saghang was born as a Chinggisid in the Ordos tribe in South Mongolia in 1604. He was eleven years old when he was granted the title Sechen Khong Tayiji in 1614, and admitted among the ruling class of ministers in his native tribe at his seventeen years of age in 1620. He was specifically honored by allowing to declaim the title of khan at the time of the accession of Rinchen Eyechi Dayiching in 1627. In 1628, Lingdan Khutughtu Khan of the Chakhar tribe came and attacked Rinchen Jinong, conquered his Ordos tribe and forced him to be a part of Chakhar army. Lingdan Khan died of smallpox on his way to a conquest of Tibet, and his power collapsed in 1634. Saghang Sechen Khong Tayiji led his colleagues out of other groups in confusion. Thus Rinchen Jinong came to his ancestral home of Jigi, and praised Saghang for his distinguished service by granting him the title of Erke Sechen Khong Tayiji, and the permit to advance in front of the great army in military affairs and to be in the middle of great hunt in peaceful affairs. He wrote his chronicle Erdeni-yin Tobchi in 1662 when he was fifty-nine years old. How long he lived is not known. His tomb is located north of Yeke Shiber in the territory of the Uushin Banner in the tribal domain of the Ordos in South Mongolia. One question remains; why he took trouble to write his chronicle? We will investigate the reason in the light of his time when the Mongols as a whole came under the ManchuCh'ing military power in the late seventeenth century. As a matter of my private concern, I published a complete Japanese translation with a commentary of Erdeni-yin Tobchi in 2004, which gives me a point of view not allowed other people.
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ICE ABSORPTION FEATURES IN NIR SPECTRA OF GALACTIC OBJECTS
TAMAMI I. MORI,TAKASHI ONAKA,ITSUKI SAKON,RYOU OHSAWA,HIDEHIRO KANEDA,MITSUYOSHI YAMAGISHI,YOKO OKADA,MASAHIRO TANAKA,TAKASHI SHIMONISHI 한국천문학회 2017 天文學論叢 Vol.32 No.1
We present results of AKARI/IRC near-infrared (NIR) slit-spectroscopy (2.5--5.0\,$\mu$m, $R \sim 100$) of Galactic sources,focusing on ice absorption features. We investigate the abundance of H$_2$O and CO$_2$ ices and other ice species (CO and XCN ices)along lines of sight towards Galactic \ion{H}{ii} regions, massive YSOs, and infrared diffuse sources. Even among those different kinds of astronomical objects,the abundance ratio of CO$_2$ to H$_2$O ices does not vary significantly,suggesting that the pathway to CO$_2$ ice formation driven by UV irradiation is not effectiveat least among the present targets.
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PROCESSING OF INTERSTELLAR MEDIUM AS DIVULGED BY AKARI
TAKASHI ONAKA,TAMAMI I. MORI,RYOU OHSAWA,ITSUKI SAKON,AARON C. BELL,MARK HAMMONDS,TAKASHI SHIMONISHI,DAISUKE ISHIHARA,HIDEHIRO KANEDA,YOKO OKADA,MASAHIRO TANAKA 한국천문학회 2017 天文學論叢 Vol.32 No.1
A wide spectral coverage from near-infrared (NIR) to far-infrared (FIR) of {\it AKARI} both for imaging and spectroscopy enablesus to efficiently study the emission from gas and dust in the interstellar medium (ISM). In particular, the Infrared Camera(IRC) onboard {\it AKARI}offers a unique opportunity to carry out sensitive spectroscopy in the NIR (2--5\,$\mu$m) for the first time from a spaceborn telescope. This spectral range contains a number of important dust bands and gas lines, such as the aromatic and aliphatic emissionbands at 3.3 and 3.4--3.5\,$\mu$m, H$_2$O and CO$_2$ ices at 3.0 and 4.3\,$\mu$m, CO, H$_2$, and \ion{H}{I} gas emission lines. In this paper we concentrate on the aromatic and aliphatic emission and ice absorption features. The balance between dust supply and destruction suggests significant dust processing takingplace as well as dust formation in the ISM. Detailed analysis of the aromatic and aliphatic bands of {\it AKARI} observations for a number of\ion{H}{ii} regions and \ion{H}{ii} region-like objectssuggests processing of carbonaceous dust in the ISM. The ice formation process canalso be studied with IRC NIR spectroscopy efficiently. In this review, dust processing in the ISM divulged by recentanalysis of {\it AKARI} data is discussed.
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