218 research outputs found

    Molecular-Cloud-Scale Chemical Composition I: Mapping Spectral Line Survey toward W51 in the 3 mm Band

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    We have conducted a mapping spectral line survey toward the Galactic giant molecular cloud W51 in the 3 mm band with the Mopra 22 m telescope in order to study an averaged chemical composition of the gas extended over a molecular cloud scale in our Galaxy. We have observed the area of 25×3025' \times 30', which corresponds to 39 pc ×\times 47 pc. The frequency ranges of the observation are 85.1 - 101.1 GHz and 107.0 - 114.9 GHz. In the spectrum spatially averaged over the observed area, spectral lines of 12 molecular species and 4 additional isotopologues are identified. An intensity pattern of the spatially-averaged spectrum is found to be similar to that of the spiral arm in the external galaxy M51, indicating that these two sources have similar chemical compositions. The observed area has been classified into 5 sub-regions according to the integrated intensity of 13^{13}CO(J=10J=1-0) (I13COI_{\rm ^{13}CO}), and contributions of the fluxes of 11 molecular lines from each sub-region to the averaged spectrum have been evaluated. For most of molecular species, 50 % or more of the flux come from the sub-regions with I13COI_{\rm ^{13}CO} from 25 K km s1^{-1} to 100 K km s1^{-1}, which does not involve active star forming regions. Therefore, the molecular-cloud-scale spectrum observed in the 3 mm band hardly represents the chemical composition of star forming cores, but mainly represents the chemical composition of an extended quiescent molecular gas. The present result constitutes a sound base for interpreting the spectra of external galaxies at a resolution of a molecular cloud scale (10\sim10 pc) or larger.Comment: Accepted for publication in Ap

    English Cafe Activity for Nursing Students to Improve English Communication Skills

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    Dicer Functions in Aquatic Species

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    Dicer is an RNase III enzyme with two catalytic subunits, which catalyzes the cleavage of double-stranded RNA to small interfering RNAs and micro-RNAs, which are mainly involved in invasive nucleic acid defense and endogenous genes regulation. Dicer is abundantly expressed in embryos, indicating the importance of the protein in early embryonic development. In addition, Dicer is thought to be involved in defense mechanism against foreign nucleic acids such as viruses. This paper will mainly focus on the recent progress of Dicer-related research and discuss potential RNA interference pathways in aquatic species

    近傍矮小銀河で探る星間分子雲の化学組成への低重元素量の影響

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    学位の種別: 課程博士審査委員会委員 : (主査)東京大学准教授 馬場 彩, 東京大学教授 吉田 直紀, 東京大学准教授 大内 正之, 国立天文台教授 長谷川 哲夫, 東京大学教授 中川 貴雄University of Tokyo(東京大学
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