Zobrazeno 1 - 10
of 1 920
pro vyhledávání: '"Muraoka K"'
Publikováno v:
Clinical, Cosmetic and Investigational Dermatology, Vol Volume 17, Pp 237-246 (2024)
Miki Iwai,1 Koichi Nakaoji,1 Kazuhiko Hamada,1 Yutaka Inaba,2 Kyoko Muraoka,2 Emi Tohsuji,2 Masatoshi Jinnin2 1Central R&D Laboratory, Pias Corporation, Kobe, Japan; 2Department of Dermatology, Wakayama Medical University, Wakayama, JapanCorresponden
Externí odkaz:
https://doaj.org/article/0b6ba87eb7654ab2a80ef9fd5b7adf00
Autor:
Demachi, F., Fukui, Y., Yamada, R. I., Tachihara, K., Hayakawa, T., Tokuda, K., Fujita, S., Kobayashi, M. I. N., Muraoka, K., Konishi, A., Tsuge, K., Onishi, T., Kawamura, A.
We investigated the giant molecular clouds (GMCs) in M74 (NGC 628), using data obtained from the PHANGS project. We applied the GMC Types according to the activity of star formation: Type I without star formation, Type II with H$\alpha$ luminosity ($
Externí odkaz:
http://arxiv.org/abs/2305.19192
Autor:
Muraoka K.
Publikováno v:
EPJ Web of Conferences, Vol 98, p 05003 (2015)
This article describes the various effects on the public conception on nuclear energy and more generally on energy policies in Japan due to the nuclear accident that occurred on 11th March 2011 at the Fukushima Dai-ichi nuclear power station, which i
Externí odkaz:
https://doaj.org/article/640019bda6924e359972a519e8984e4d
NGC 253 is a starburst galaxy of SAB(s)c type with increasing interest because of its high activity at unrivaled closeness. Its energetic event is manifested as the vertical gas features in its central molecular zone, for which stellar feedback was p
Externí odkaz:
http://arxiv.org/abs/2106.01653
Autor:
Koda, J., Sawada, T., Sakamoto, K., Hirota, A., Egusa, F., Boissier, S., Calzetti, D., Meyer, J. Donovan, Elmegreen, B. G., de Paz, A. Gil, Harada, N., Ho, L. C., Kobayashi, M. I. N., Kuno, N., Martin, S., Muraoka, K., Nakanishi, K., Scoville, N., Seibert, M., Vlahakis, C., Watanabe, Y.
We present spatial variations of the CO J=2-1/1-0 line ratio in M83 using Total Power array data from ALMA. While the intensities of these two lines correlate tightly, the ratio varies over the disk, with a disk average ratio of 0.69, and shows the g
Externí odkaz:
http://arxiv.org/abs/2001.11043
Autor:
Sano, H., Matsumura, H., Yamane, Y., Maggi, P., Fujii, K., Tsuge, K., Tokuda, K., Alsaberi, R. Z. E., Filipovic, M. D., Maxted, N., Rowell, G., Uchida, H., Tanaka, T., Muraoka, K., Takekoshi, T., Onishi, T., Kawamura, A., Minamidani, T., Mizuno, N., Yamamoto, H., Tachihara, K., Inoue, T., Inutsuka, S., Voisin, F., Tothill, N. F. H., Sasaki, M., McClure-Griffiths, N. M., Fukui, Y.
RX J0046.5$-$7308 is a shell-type supernova remnant (SNR) in the Small Magellanic Cloud (SMC). We carried out new $^{12}$CO($J$ = 1-0, 3-2) observations toward the SNR using Mopra and the Atacama Submillimeter Telescope Experiment. We found eight mol
Externí odkaz:
http://arxiv.org/abs/1904.04836
Akademický článek
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Akademický článek
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Autor:
Iono, D., Hatsukade, B., Kohno, K., Kawabe, R., Ikarashi, S., Ichikawa, K., Kodama, T., Motohara, K., Nakajima, T., Nakanishi, K., Ohta, K., Ota, K., Saito, T., Suzuki, K., Tadaki, K., Tamura, Y., Ueda, J., Umehata, H., Yabe, K., Yoshida, T., Yuma, S., Kuno, N., Takano, S., Iwashita, H., Handa, K., Higuchi, A., Hirota, A., Ishikawa, S., Kimura, K., Maekawa, J., Mikoshiba, H., Miyazawa, C., Miyazawa, K., Muraoka, K., Ogawa, H., Onodera, S., Saito, Y., Sakai, T., Takahashi, S., Yun, M. S.
We present initial results from the CO survey toward high redshift galaxies using the Nobeyama 45m telescope. Using the new wide bandwidth spectrometer equipped with a two-beam SIS receiver, we have robust new detections of three high redshift (z=1.6
Externí odkaz:
http://arxiv.org/abs/1206.3840
Autor:
Komugi, S., Tosaki, T., Kohno, K., Tsukagoshi, T., Nakanishi, K., Sawada, T., Kawabe, R., Ezawa, H., Kuno, N., Onodera, S., Tamura, Y., Wilson, G. W., Yun, M. S., Scott, K., Perera, T. A., Austermann, J. E., Hughes, D. H., Aretxaga, I., Tanaka, K., Muraoka, K., Miura, R., Egusa, F.
We present wide-field 1.1 mm continuum imaging of the nearby spiral galaxy M 33, conducted with the AzTEC bolometer camera on ASTE. We show that the 1.1 mm flux traces the distribution of dust with T ~20 K. Combined with far-infrared imaging at 160um
Externí odkaz:
http://arxiv.org/abs/1106.2166