Zobrazeno 1 - 10
of 387
pro vyhledávání: '"Mito, H"'
Autor:
Semkov, E. H., Peneva, S. P., Munari, U., Dennefeld, M., Mito, H., Dimitrov, D. P., Ibryamov, S., Stoyanov, K. A.
We carried out BVRI CCD photometric observations in the field of V582 Aur from 2009 August to 2013 February. We acquired high-, medium-, and low-resolution spectroscopy of V582 Aur during this period. To study the pre-outburst variability of the targ
Externí odkaz:
http://arxiv.org/abs/1306.6647
Autor:
Jose, Jessy, Pandey, A. K., Ogura, K., Samal, M. R., Ojha, D. K., Bhatt, B. C., Chauhan, N., Eswaraiah, C., Mito, H., Kobayashi, N., Yadav, R. K.
Publikováno v:
MNRAS, 2012, Volume 424, Issue 4, pp. 2486-2503
We present the analyses of the stellar contents associated with the HII region Sh2-252 using UBVRI photometry, slit and slitless spectroscopy along with the NIR data from 2MASS for an area ~1 degree x 1 degree. We studied the sub-regions of Sh2-252 w
Externí odkaz:
http://arxiv.org/abs/1212.6594
Autor:
Sharma, Saurabh, Pandey, A. K., Pandey, J. C., Chauhan, N., Ogura, K., Ojha, D. K., Borrissova, J., Mito, H., Verdugo, T., Bhatt, B. C.
Publikováno v:
2012 PASJ, Vol 64 No. 6
We present a multiwavelength study of the NGC 281 complex which contains the young cluster IC 1590 at the center, using deep wide-field optical UBVI_c photometry, slitless spectroscopy along with archival data sets in the near-infrared (NIR) and X-ra
Externí odkaz:
http://arxiv.org/abs/1204.2897
The aim of this paper is to present the results of photometric investigations of the central cluster of the W5 E region as well as a follow-up study of the triggered star formation in and around bright-rimmed clouds (BRCs). We have carried out wide f
Externí odkaz:
http://arxiv.org/abs/1103.3396
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
Autor:
Jose, Jessy, Pandey, A. K., Ojha, D. K., Ogura, K., Chen, W. P., Bhatt, B. C., Ghosh, S. K., Mito, H., Maheswar, G., Sharma, Saurabh
We present $UBVI_c$ CCD photometry of the young open cluster Stock 8 with the aim to study the basic properties and star formation scenario in this region. The radius of the cluster is found to be $\sim 6^{\prime}$ ($\sim 3.6$ pc) and the reddening w
Externí odkaz:
http://arxiv.org/abs/0712.2159
Autor:
Urata, Y., Huang, K. Y., Qiu, Y. L., Hu, J., Kuo, P. H., Tamagawa, T., Ip, W. H., Kinoshita, D., Fukushi, H., Isogai, M., Miyata, T., Nakada, Y., Aoki, T., Soyano, T., Tarusawa, K., Mito, H., Onda, K., Ibrahimov, M., Pozanenko, A., Makishima, K.
Publikováno v:
Astrophys.J.655:L81-L84,2007
Observations of the optical afterglow of GRB 041006 with the Kiso Observatory 1.05 m Schmidt telescope, the Lulin Observatory 1.0 m telescope and the Xinglong Observatory 0.6 m telescope. Three-bands (B, V and R) of photometric data points were obtai
Externí odkaz:
http://arxiv.org/abs/astro-ph/0612623
Autor:
Huang, K. Y., Urata, Y., Kuo, P. H., Ip, W. H., Ioka, K., Aoki, T., Chen, C. W., Chen, W. P., Isogai, M., Lin, H. C., Makishima, K., Mito, H., Miyata, T., Nakada, Y., Nishiura, S., Onda, K., Qiu, Y., Soyano, T., Tamagawa, T., Tarusawa, K., Tashiro, M., Yoshioka, T.
Publikováno v:
Astrophys.J.654:L25-L28,2006
Multi-wavelength B, V, R, I observations of the optical afterglow of GRB 050319 were performed by the 1.05-m telescope at Kiso Observatory and the 1.0-m telescope at Lulin Observatory from 1.31 hours to 9.92 hours after the burst. Our R band lightcur
Externí odkaz:
http://arxiv.org/abs/astro-ph/0611323