Zobrazeno 1 - 10
of 448
pro vyhledávání: '"Yamamura, I"'
Autor:
Scicluna, P., Kemper, F., McDonald, I., Srinivasan, S., Trejo, A., Wallström, S. H. J., Wouterloot, J. G. A., Cami, J., Greaves, J., He, Jinhua, Hoai, D. T., Kim, Hyosun, Jones, O. C., Shinnaga, H., Clark, C. J. R., Dharmawardena, T., Holland, W., Imai, H., van Loon, J. Th., Menten, K. M., Wesson, R., Chawner, H., Feng, S., Goldman, S., Liu, F. C., MacIsaac, H., Tang, J., Zeegers, S., Amada, K., Antoniou, V., Bemis, A., Boyer, M. L., Chapman, S., Chen, X., Cho, S. -H., Cui, L., Dell'Agli, F., Friberg, P., Fukaya, S., Gomez, H., Gong, Y., Hadjara, M., Haswell, C., Hirano, N., Hony, S., Izumiura, H., Jeste, M., Jiang, X., Kaminski, T., Keaveney, N., Kim, J., Kraemer, K. E., Kuan, Y. -J., Lagadec, E., Lee, C. F., Li, D., Liu, S. -Y., Liu, T., de Looze, I., Lykou, F., Maraston, C., Marshall, J. P., Matsuura, M., Min, C., Otsuka, M., Oyadomari, M., Parsons, H., Patel, N. A., Peeters, E., Pham, T. A., Qiu, J., Randall, S., Rau, G., Redman, M. P., Richards, A. M. S., Serjeant, S., Shi, C., Sloan, G. C., Smith, M. W. L., Suh, K. -W., Toalá, J. A., Uttenthaler, S., Ventura, P., Wang, B., Yamamura, I., Yang, T., Yun, Y., Zhang, F., Zhang, Y., Zhao, G., Zhu, M., Zijlstra, A. A.
The Nearby Evolved Stars Survey (NESS) is a volume-complete sample of $\sim$850 Galactic evolved stars within 3\,kpc at (sub-)mm wavelengths, observed in the CO $J = $ (2$-$1) and (3$-$2) rotational lines, and the sub-mm continuum, using the James Cl
Externí odkaz:
http://arxiv.org/abs/2110.12562
Autor:
Roelfsema, P. R., Shibai, H., Armus, L., Arrazola, D., Audard, M., Audley, M. D., Bradford, C. M., Charles, I., Dieleman, P., Doi, Y., Duband, L., Eggens, M., Evers, J., Funaki, I., Gao, J. R., Giard, M., Fernández, A. di Giorgio L. M. González, Griffin, M., Helmich, F. P., Hijmering, R., Huisman, R., Ishihara, D., Isobe, N., Jackson, B., Jacobs, H., Jellema, W., Kamp, I., Kaneda, H., Kawada, M., Kemper, F., Kerschbaum, F., Khosropanah, P., Kohno, K., Kooijman, P. P., Krause, O., van der Kuur, J., Kwon, J., Laauwen, W. M., de Lange, G., Larsson, B., van Loon, D., Madden, S. C., Matsuhara, H., Najarro, F., Nakagawa, T., Naylor, D., Ogawa, H., Onaka, T., Oyabu, S., Poglitsch, A., Reveret, V., Rodriguez, L., Spinoglio, L., Sakon, I., Sato, Y., Shinozaki, K., Shipman, R., Sugita, H., Suzuki, T., van der Tak, F. F. S., Redondo, J. Torres, Wada, T., Wang, S. Y., Wafelbakker, C. K., van Weers, H., Withington, S., Vandenbussche, B., Yamada, T., Yamamura, I.
Measurements in the infrared wavelength domain allow us to assess directly the physical state and energy balance of cool matter in space, thus enabling the detailed study of the various processes that govern the formation and early evolution of stars
Externí odkaz:
http://arxiv.org/abs/1803.10438
Autor:
Ueta, T., Ladjal, D., Exter, K. M., Otsuka, M., Szczerba, R., Siódmiak, N., Aleman, I., van Hoof, P. A. M., Kastner, J. H., Montez, R., McDonald, I., Wittkowski, M., Sandin, C., Ramstedt, S., De Marco, O., Villaver, E., Chu, Y. -H., Vlemmings, W., Izumiura, H., Sahai, R., Lopez, J. A., Balick, B., Zijlstra, A., Tielens, A. G. G. M., Rattray, R. E., Behar, E., Blackman, E. G., Hebden, K., Hora, J. L., Murakawa, K., Nordhaus, J., Nordon, R., Yamamura, I
This is the first of a series of investigations into far-IR characteristics of 11 planetary nebulae (PNs) under the Herschel Space Observatory Open Time 1 program, Herschel Planetary Nebula Survey (HerPlaNS). Using the HerPlaNS data set, we look into
Externí odkaz:
http://arxiv.org/abs/1403.2494
Autor:
Sorahana, S., Yamamura, I.
We investigate variations in the strengths of three molecular bands, CH4 at 3.3 um, CO at 4.6 um and CO2 at 4.2 um, in 16 brown dwarf spectra obtained by AKARI. Spectral features are examined along the sequence of source classes from L1 to T8. We fin
Externí odkaz:
http://arxiv.org/abs/1210.3828
Autor:
Yamauchi, C., Fujishima, S., Ikeda, N., Inada, K., Katano, M., Kataza, H., Makiuti, S., Matsuzaki, K., Takita, S., Yamamoto, Y., Yamamura, I.
Publikováno v:
2011PASP..123..852Y
The AKARI All-Sky Catalogues are an important infrared astronomical database for next-generation astronomy that take over the IRAS catalog. We have developed an online service, AKARI Catalogue Archive Server (AKARI-CAS), for astronomers. The service
Externí odkaz:
http://arxiv.org/abs/1107.5385
Autor:
Oyabu, S., Ishihara, D., Malkan, M., Matsuhara, H., Wada, T., Nakagawa, T., Ohyama, Y., Toba, Y., Onaka, T., Takita, S., Kataza, H., Yamamura, I., Shirahata, M.
We present a new sample of active galactic nuclei (AGNs) identified using the catalog of the AKARI Mid-infrared(MIR) All-Sky Survey. Our MIR search has an advantage in detecting AGNs that are obscured at optical wavelengths due to extinction. We firs
Externí odkaz:
http://arxiv.org/abs/1103.2453
Autor:
Ita, Y., Matsuura, M., Ishihara, D., Oyabu, S., Takita, S., Kataza, H., Yamamura, I., Matsunaga, N., Tanabe, T., Nakada, Y., Fujiwara, H., Wada, T., Onaka, T., Matsuhara, H.
Results: We found that the (B-V) v.s. (V-S9W) color-color diagram is useful to identify the stars with infrared excess emerged from circumstellar envelopes/disks. Be stars with infrared excess are well separated from other types of stars in this diag
Externí odkaz:
http://arxiv.org/abs/1003.1370
Autor:
Ita, Y., Onaka, T., Tanabe, T., Matsunaga, N., Matsuura, M., Yamamura, I., Nakada, Y., Izumiura, H., Ueta, T., Mito, H., Fukushi, H., Kato, D.
We carried out a near- to mid-infrared imaging and spectroscopic observations of the patchy areas in the Small Magellanic Cloud using the Infrared Camera on board AKARI. Two 100 arcmin2 areas were imaged in 3.2, 4.1, 7, 11, 15, and 24 um and also spe
Externí odkaz:
http://arxiv.org/abs/1001.1791
Autor:
Ueta, T., Stencel, R. E., Yamamura, I., Geise, K. M., Karska, A., Izumiura, H., Nakada, Y., Matsuura, M., Ita, Y., Tanabe, T., Fukushi, H., Matsunaga, N., Mito, H., Speck, A. K.
The circumstellar dust shells of intermediate initial-mass (about 1 to 8 solar masses) evolved stars are generated by copious mass loss during the asymptotic giant branch phase. The density structure of their circumstellar shell is the direct evidenc
Externí odkaz:
http://arxiv.org/abs/0911.4918
Autor:
Matsunaga, N., Mito, H., Nakada, Y., Fukushi, H., Tanabé, T., Ita, Y., Izumiura, H., Matsuura, M., Ueta, T., Yamamura, I.
Publikováno v:
Publ.Astron.Soc.Jap.60:415-428,2008
We report the observations of 12 globular clusters with the AKARI/FIS. Our goal is to search for emission from the cold dust within clusters. We detect diffuse emissions toward NGC 6402 and 2808, but the IRAS 100-micron maps show the presence of stro
Externí odkaz:
http://arxiv.org/abs/0809.2853