Zobrazeno 1 - 10
of 28
pro vyhledávání: '"Horachi, H."'
Autor:
Sano, H., Fukuda, T., Yoshiike, S., Sato, J., Horachi, H., Kuwahara, T., Torii, K., Hayakawa, T., Tanaka, T., Matsumoto, H., Inoue, T., Yamazaki, R., Inutsuka, S., Kawamura, A., Yamamoto, H., Okuda, T., Tachihara, K., Mizuno, N., Onishi, T., Mizuno, A., Acero, F., Fukui, Y.
We have carried out a spectral analysis of the Suzaku X-ray data in the 0.4-12 keV range toward the shell-type very-high-energy {\gamma}-ray supernova remnant RX J1713.7-3946. The aims of this analysis are to estimate detailed X-rays spectral propert
Externí odkaz:
http://arxiv.org/abs/1401.7418
Autor:
Sano, H., Tanaka, T., Torii, K., Fukuda, T., Yoshiike, S., Sato, J., Horachi, H., Kuwahara, T., Hayakawa, T., Matsumoto, H., Inoue, T., Yamazaki, R., Inutsuka, S., Kawamura, A., Tachihara, K., Yamamoto, H., Okuda, T., Mizuno, N., Onishi, T., Mizuno, A., Fukui, Y.
RX J1713.7-3946 is the most remarkable very-high-energy \gamma-ray supernova remnant which emits synchrotron X-rays without thermal features. We made a comparative study of CO, HI and X-rays in order to better understand the relationship between the
Externí odkaz:
http://arxiv.org/abs/1304.7722
Autor:
Fukui, Y., Sano, H., Sato, J., Torii, K., Horachi, H., Hayakawa, T., McClure-Griffiths, N. M., Rowell, G., Inoue, T., Inutsuka, S., Kawamura, A., Yamamoto, H., Okuda, T., Mizuno, N., Onishi, T., Mizuno, A., Ogawa, H.
RX J1713.7$-$3946 is the most remarkable TeV $\gamma$-ray SNR which emits $\gamma$-rays in the highest energy range. We made a new combined analysis of CO and \ion{H}{1} in the SNR and derived the total protons in the interstellar medium (ISM). We ha
Externí odkaz:
http://arxiv.org/abs/1107.0508
Autor:
Sano, H., Sato, J., Horachi, H., Moribe, N., Yamamoto, H., Hayakawa, T., Torii, K., Kawamura, A., Okuda, T., Mizuno, N., Onishi, T., Maezawa, H., Inoue, T., Inutsuka, S., Tanaka, T., Matsumoto, H., Mizuno, A., Ogawa, H., Stutzki, J., Bertoldi, F., Anderl, S., Bronfman, L., Koo, B. -C., Burton, M. G., Benz, A. O., Fukui, Y.
RX J1713.7-3946 is one of the TeV {\gamma}-ray supernova remnants (SNRs) emitting synchrotron X rays. The SNR is associated with molecular gas located at ~1 kpc. We made new molecular observations toward the dense cloud cores, peaks A, C and D, in th
Externí odkaz:
http://arxiv.org/abs/1005.3409
Autor:
Sano, H., Fukuda, T., Yoshiike, S., Sato, J., Horachi, H., Kuwahara, T., Torii, K., Hayakawa, T., Tanaka, T., Matsumoto, H., Inoue, T., Yamazaki, R., Inutsuka, S., Kawamura, A., Yamamoto, H., Okuda, T., Tachihara, K., Mizuno, N., Onishi, T., Mizuno, A., Acero, F., Fukui, Y.
We have carried out a spectral analysis of the Suzaku X-ray data in the 0.4-12 keV range toward the shell-type very-high-energy ��-ray supernova remnant RX J1713.7-3946. The aims of this analysis are to estimate detailed X-rays spectral propertie
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ba29d1b4fef82550f309abe54a32c2cb
Autor:
Sano, H., Tanaka, T., Torii, K., Fukuda, T., Yoshiike, S., Sato, J., Horachi, H., Kuwahara, T., Hayakawa, T., Matsumoto, H., Inoue, T., Yamazaki, R., Inutsuka, S., Kawamura, A., Tachihara, K., Yamamoto, H., Okuda, T., Mizuno, N., Onishi, T., Mizuno, A., Fukui, Y.
RX J1713.7-3946 is the most remarkable very-high-energy ��-ray supernova remnant which emits synchrotron X-rays without thermal features. We made a comparative study of CO, HI and X-rays in order to better understand the relationship between the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cb22424365e05caaf39b2f7f1d688d84
Autor:
Fukui, Y., Sano, H., Sato, J., Torii, K., Horachi, H., Hayakawa, T., McClure-Griffiths, N. M., Rowell, G., Inoue, T., Inutsuka, S., Kawamura, A., Yamamoto, H., Okuda, T., Mizuno, N., Onishi, T., Mizuno, A., Ogawa, H.
RX J1713.7$-$3946 is the most remarkable TeV $��$-ray SNR which emits $��$-rays in the highest energy range. We made a new combined analysis of CO and \ion{H}{1} in the SNR and derived the total protons in the interstellar medium (ISM). We ha
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::eea8a34ddb03cfed3ceaa040bf35fe6a
Autor:
Sano, H., Sato, J., Horachi, H., Moribe, N., Yamamoto, H., Hayakawa, T., Torii, K., Kawamura, A., Okuda, T., Mizuno, N., Onishi, T., Maezawa, H., Inoue, T., Inutsuka, S., Tanaka, T., Matsumoto, H., Mizuno, A., Ogawa, H., Stutzki, J., Bertoldi, F., Anderl, S., Bronfman, L., Koo, B. -C., Burton, M. G., Benz, A. O., Fukui, Y.
RX J1713.7-3946 is one of the TeV ��-ray supernova remnants (SNRs) emitting synchrotron X rays. The SNR is associated with molecular gas located at ~1 kpc. We made new molecular observations toward the dense cloud cores, peaks A, C and D, in the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::231744c56bb614bcd02dea9be67df41b
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Akademický článek
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