Zobrazeno 1 - 10
of 1 560
pro vyhledávání: '"Nakamura O."'
Autor:
Silva A. Ferreira da, Silva T. Souza da, Nakamura O., d?Aguiar Neto M.M.F., Pepe I., Roman L. S., Veje E.
Publikováno v:
Materials Research, Vol 4, Iss 1, Pp 23-26 (2001)
Thermal diffusivity and optical absorption have been investigated for porous silicon, at room temperature, using photoacoustic spectroscopy. The experimental results obtained conform well with the existing studies recently published. The value obtain
Externí odkaz:
https://doaj.org/article/185904d26e324ad2b7db55e23e47ca7a
Autor:
Nakanishi, H. *, Yamanaka, K., Tokunaga, S., Ozeki, T., Homma, Y., Ohtsu, H., Ishii, Y., Nakajima, N., Yamamoto, T., Emoto, M., Ohsuna, M., Ito, T., Imazu, S., Nonomura, M., Yoshida, M., Ogawa, H., Maeno, H., Aoyagi, M., Yokota, M., Inoue, T., Nakamura, O., Abe, S., Urushidani, S.
Publikováno v:
In Fusion Engineering and Design April 2021 165
Publikováno v:
Astrophys.J.705:245-254,2009
A bulge-disk decomposition is made for 737 spiral and lenticular galaxies drawn from a SDSS galaxy sample for which morphological types are estimated. We carry out the bulge-disk decomposition using the growth curve fitting method. It is found that b
Externí odkaz:
http://arxiv.org/abs/0908.4312
Publikováno v:
Mon.Not.Roy.Astron.Soc.368:1871-1879,2006
We examine the evolutionary status of luminous, star-forming galaxies in intermediate-redshift clusters by considering their star formation rates and the chemical and ionsiation properties of their interstellar emitting gas. Our sample consists of 17
Externí odkaz:
http://arxiv.org/abs/astro-ph/0603640
Publikováno v:
Mon.Not.Roy.Astron.Soc.369:891-908,2006
We derive oxygen abundances for a sample of 40 luminous (M_{B} < -19), star-forming, mostly disk, field galaxies with redshifts in the range 0.2 < z < 0.8$, with a median of = 0.45. Oxygen abundances, relative to hydrogen, of the interstellar emi
Externí odkaz:
http://arxiv.org/abs/astro-ph/0603639
Autor:
Nakamura, O., Aragon-Salamanca, A., Milvang-Jensen, B., Arimoto, N., Ikuta, C., Bamford, S. P.
Publikováno v:
Mon.Not.Roy.Astron.Soc.366:144-162,2006
We have carried out spectroscopic observations in 4 cluster fields using Subaru's FOCAS multi-slit spectrograph and obtained spectra for 103 bright disk field and cluster galaxies at $0.06 \le z \le 1.20$. Seventy-seven of these show emission lines,
Externí odkaz:
http://arxiv.org/abs/astro-ph/0511831
Autor:
Zehavi, I., Zheng, Z., Weinberg, D. H., Frieman, J. A., Berlind, A. A., Blanton, M. R., Scoccimarro, R., Sheth, R. K., Strauss, M. A., Kayo, I., Suto, Y., Fukugita, M., Nakamura, O., Bahcall, N. A., Brinkmann, J., Gunn, J. E., Hennessy, G. S., Ivezic, Z., Knapp, G. R., Loveday, J., Meiksin, A., Schlegel, D. J., Schneider, D. P., Szapudi, I., Tegmark, M., Vogeley, M. S., York, D. G.
Publikováno v:
Astrophys.J.630:1-27,2005
We study the luminosity and color dependence of the galaxy 2-point correlation function in the Sloan Digital Sky Survey, starting from a sample of 200,000 galaxies over 2500 deg^2. We concentrate on the projected correlation function w(r_p), which is
Externí odkaz:
http://arxiv.org/abs/astro-ph/0408569
Autor:
Collaboration, QCD-TARO, de Forcrand, Ph., Perez, M. Garcia, Hashimoto, T., Hioki, S., Katayama, R., Matsufuru, H., Nakamura, O. Miyamura A., Stamatescu, I. -O., Takaishi, T., Umeda, T.
Publikováno v:
Nucl.Phys.Proc.Suppl. 83 (2000) 411-413
We present results for mesonic propagators in temporal and spatial directions at T below and above the deconfining transition in quenched QCD. Anisotropic lattices are used to get enough information in the temporal direction. We use the Wilson fermio
Externí odkaz:
http://arxiv.org/abs/hep-lat/9911001
Autor:
Takenouchi, A., Otomo, T., Niwa, K., Sakai, M., Saito, Y., Kirigane, T., Kosaka, M., Michimura, S., Hasegawa, S., Nakamura, O.
Publikováno v:
In Journal of Crystal Growth 15 June 2017 468:701-704
Autor:
Yabuki, K., Hirama, H., Aoki, N., Sakai, M., Saito, Y., Higuchi, K., Kitajima, A., Hasegawa, S., Nakamura, O.
Publikováno v:
In Journal of Crystal Growth 15 June 2017 468:714-717