Two Possible Soft X-Ray Counterparts to Gamma-Ray Burst Sources

K.Hurley K.Hurley, T.Murakami T.Murakami, P.Li P.Li, A.Smette A.Smette, Y.Ogasaka Y.Ogasaka, G.Ricker G.Ricker, N.Kawai N.Kawai, M.Matsuoka M.Matsuoka, M.Yamauchi M.Yamauchi, A.Yoshida A.Yoshida, J.Nishimura J.Nishimura, Kenji Yoshida, C.Kouvelitou C.Kouvelitou

研究成果: Article

元の言語English
ページ(範囲)173-175
ジャーナルProc.of all-Sky X-ray Observation in the Next Decade
出版物ステータスPublished - 1997 1 1

これを引用

K.Hurley, K. H., T.Murakami, T. M., P.Li, P. L., A.Smette, A. S., Y.Ogasaka, Y. O., G.Ricker, G. R., N.Kawai, N. K., M.Matsuoka, M. M., M.Yamauchi, M. Y., A.Yoshida, A. Y., J.Nishimura, J. N., Yoshida, K., & C.Kouvelitou, C. K. (1997). Two Possible Soft X-Ray Counterparts to Gamma-Ray Burst Sources. Proc.of all-Sky X-ray Observation in the Next Decade, 173-175.