Zobrazeno 1 - 10
of 1 368
pro vyhledávání: '"Soong, Y."'
Autor:
Miller, M. C., Lamb, F. K., Dittmann, A. J., Bogdanov, S., Arzoumanian, Z., Gendreau, K. C., Guillot, S., Harding, A. K., Ho, W. C. G., Lattimer, J. M., Ludlam, R. M., Mahmoodifar, S., Morsink, S. M., Ray, P. S., Strohmayer, T. E., Wood, K. S., Enoto, T., Foster, R., Okajima, T., Prigozhin, G., Soong, Y.
Publikováno v:
ApJL 2019, 887, L24
Neutron stars are not only of astrophysical interest, but are also of great interest to nuclear physicists, because their attributes can be used to determine the properties of the dense matter in their cores. One of the most informative approaches fo
Externí odkaz:
http://arxiv.org/abs/1912.05705
Autor:
Keek, L., Arzoumanian, Z., Bult, P., Cackett, E. M., Chakrabarty, D., Chenevez, J., Fabian, A. C., Gendreau, K. C., Guillot, S., Güver, T., Homan, J., Jaisawal, G. K., Lamb, F. K., Ludlam, R. M., Mahmoodifar, S., Markwardt, C. B., Miller, J. M., Prigozhin, G., Soong, Y., Strohmayer, T. E., Wolff, M. T.
Publikováno v:
The Astrophysical Journal Letters, Volume 855, Issue 1, article id. L4, 6 pp. (2018)
Accretion disks around neutron stars regularly undergo sudden strong irradiation by Type I X-ray bursts powered by unstable thermonuclear burning on the stellar surface. We investigate the impact on the disk during one of the first X-ray burst observ
Externí odkaz:
http://arxiv.org/abs/1808.06441
Microwave-accelerated regeneration of a non-aqueous slurry for energy-efficient carbon sequestration
Autor:
Ji, T., Zhai, H., Wang, C., Culp, J., Marin, C.M., Paudel, H.P., Wilfong, W.C., Duan, Y., Xia, R., Jiao, F., Kail, B., Wang, Q., Soong, Y., Shi, F., Gray, M.
Publikováno v:
In Materials Today Sustainability November 2022 19
Autor:
Nakajima, H., Maeda, Y., Uchida, H., Tanaka, T., Tsunemi, H., Hayashida, K., Tsuru, T. G., Dotani, T., Nagino, R., Inoue, S., Ozaki, M., Tomida, H., Natsukari, C., Ueda, S., Mori, K., Yamauchi, M., Hatsukade, I., Nishioka, Y., Sakata, M., Beppu, T., Honda, D., Nobukawa, M., Hiraga, J. S., Kohmura, T., Murakami, H., Nobukawa, K. K., Bamba, A., Doty, J. P., Iizuka, R., Sato, T., Kurashima, S., Nakaniwa, N., Asai, R., Ishida, M., Mori, H., Soong, Y., Okajima, T., Serlemitsos, P., Tawara, Y., Mitsuishi, I., Ishibashi, K., Tamura, K., Hayashi, T., Furuzawa, A., Sugita, S., Miyazawa, T., Awaki, H., Miller, E. D., Yamaguchi, H.
We describe the in-orbit performance of the soft X-ray imaging system consisting of the Soft X-ray Telescope and the Soft X-ray Imager aboard Hitomi. Verification and calibration of imaging and spectroscopic performance are carried out making the bes
Externí odkaz:
http://arxiv.org/abs/1709.08829
Autor:
Done, C., Tsujimoto, M., Cackett, E., Herder, J. W. den, Dotani, T., Enoto, T., Ferrigno, C., Kallman, T., Kohmura, T., Laurent, P., Miller, J., Mineshige, S., Mori, H., Nakazawa, K., Paerels, F., Sakurai, S., Soong, Y., Sugita, S., Takahashi, H., Tamagawa, T., Tanaka, Y., Terada, Y., Uno, S.
There is still 10-20% uncertainty on the neutron star (NS) mass-radius relation. These uncertainties could be reduced by an order of magnitude through an unambiguous measure of M/R from the surface redshift of a narrow line, greatly constraining the
Externí odkaz:
http://arxiv.org/abs/1412.1164
Autor:
Terada, Y., Mihara, T., Nakajima, M., Suzuki, M., Isobe, N., Makishima, K., Takahashi, H., Enoto, T., Kokubun, M., Kitaguchi, T., Naik, S., Dotani, T., Nagase, F., Tanaka, T., Watanabe, S., Kitamoto, S., Sudoh, K., Yoshida, A., Nakagawa, Y., Sugita, S., Kohmura, T., Kotani, T., Yonetoku, D., Angelini, L., Cottam, J., Mukai, K., Kelley, R., Soong, Y., Bautz, M., Kissel, S., Doty, J.
Publikováno v:
Astrophys.J.648:L139-L142,2006
The binary X-ray pulsar A0535+262 was observed with the Suzaku X-ray observatory, on 2005 September 14 for a net exposure of 22 ksec. The source was in a declining phase of a minor outburst, exhibiting 3--50 keV luminosity of about $3.7 \times 10^{35
Externí odkaz:
http://arxiv.org/abs/astro-ph/0607659
We present a conceptual design for a new X-ray all sky monitor (ASM). Compared with previous ASMs, its salient features are: (1) it has a focusing capability that increases the signal to background ratio by a factor of 3; (2) it has a broad-band widt
Externí odkaz:
http://arxiv.org/abs/astro-ph/9704007
Akademický článek
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Publikováno v:
Acta Montanistica Slovaca, Vol 3, Iss 3, Pp 393-400 (1998)
V èlánku sú diskutované niektoré technické aspekty triboelektrostatickej separácie a výs-ledky aplikácie tohto postupu pri úprave troch typov uhlia, konkrétne energetického uhlia z Cíg¾a, Handlovej a Novák. Bolo zistené, e úèinnos s
Externí odkaz:
https://doaj.org/article/49984ef09e4240b68aa890d0dd824385