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Your search keyword '"Lu, F.J."' showing total 27 results
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27 results on '"Lu, F.J."'

2. Accretion torque reversals in GRO J1008-57 revealed by Insight-HXMT

Author

Wang, W., Tang, Y.M., Tuo, Y.L., Epili, P.R., Zhang, S.N., Song, L.M., Lu, F.J., Qu, J.L., Zhang, S., Ge, M.Y., Huang, Y., Li, B., Bu, Q.C., Cai, C., Cao, X.L., Chang, Z., Chen, L., Chen, T.X., Chen, Y.B., Chen, Y., Chen, Y.P., Cui, W.W., Du, Y.Y., Gao, G.H., Gao, H., Gu, Y.D., Guan, J., Guo, C.C., Han, D.W., Huo, J., Jia, S.M., Jiang, W.C., Jin, J., Kong, L.D., Li, C.K., Li, G., Li, T.P., Li, W., Li, X., Li, X.B., Li, X.F., Li, Z.W., Liang, X.H., Liao, J.Y., Liu, B.S., Liu, C.Z., Liu, H.X., Liu, H.W., Lu, X.F., Luo, Q., Luo, T., Ma, R.C., Ma, X., Meng, B., Nang, Y., Nie, J.Y., Ou, G., Ren, X.Q., Sai, N., Song, X.Y., Sun, L., Tao, L., Wang, C., Wang, L.J., Wang, P.J., Wang, W.S., Wang, Y.S., Wen, X.Y., Wu, B.Y., Wu, B.B., Wu, M., Xiao, G.C., Xiao, S., Xiong, S.L., Xu, Y.P., Yang, R.J., Yang, S., Yang, J.J., Yang, Y.J., Yi, B.B., Yin, Q.Q., You, Y., Zhang, F., Zhang, H.M., Zhang, J., Zhang, P., Zhang, W., Zhang, W.C., Zhang, Y.F., Zhang, Y.H., Zhao, H.S., Zhao, X.F., Zheng, S.J., Zheng, Y.G., and Zhou, D.K.

Published
2021
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3. Insight-HXMT insight into switch of the accretion mode: The case of the X-ray pulsar 4U 1901+03

Author

Tuo, Y.L., Ji, L., Tsygankov, S.S., Mihara, T., Song, L.M., Ge, M.Y., Nabizadeh, A., Tao, L., Qu, J.L., Zhang, Y., Zhang, S., Zhang, S.N., Bu, Q.C., Chen, L., Xu, Y.P., Cao, X.L., Chen, Y., Liu, C.Z., Cai, C., Chang, Z., Chen, G., Chen, T.X., Chen, Y.B., Chen, Y.P., Cui, W., Cui, W.W., Deng, J.K., Dong, Y.W., Du, Y.Y., Fu, M.X., Gao, G.H., Gao, H., Gao, M., Gu, Y.D., Guan, J., Guo, C.C., Han, D.W., Huang, Y., Huo, J., Jia, S.M., Jiang, L.H., Jiang, W.C., Jin, J., Jin, Y.J., Kong, L.D., Li, B., Li, C.K., Li, G., Li, M.S., Li, T.P., Li, W., Li, X., Li, X.B., Li, X.F., Li, Y.G., Li, Z.W., Liang, X.H., Liao, J.Y., Liu, B.S., Liu, G.Q., Liu, H.W., Liu, X.J., Liu, Y.N., Lu, B., Lu, F.J., Lu, X.F., Luo, Q., Luo, T., Ma, X., Meng, B., Nang, Y., Nie, J.Y., Ou, G., Sai, N., Shang, R.C., Song, X.Y., Sun, L., Tan, Y., Wang, C., Wang, G.F., Wang, J., Wang, W.S., Wang, Y.S., Wen, X.Y., Wu, B.Y., Wu, B.B., Wu, M., Xiao, G.C., Xiao, S., Xiong, S.L., Yang, J.W., Yang, S., Yang, Y.J., Yi, Q.B., Yin, Q.Q., You, Y., Zhang, A.M., Zhang, C.M., Zhang, F., Zhang, H.M., Zhang, J., Zhang, T., Zhang, W., Zhang, W.C., Zhang, W.Z., Zhang, Y.F., Zhang, Y.J., Zhang, Y.H., Zhang, Z., Zhang, Z.L., Zhao, H.S., Zhao, X.F., Zheng, S.J., Zheng, Y.G., Zhou, D.K., Zhou, J.F., Zhu, Y.X., Zhu, Y., and Zhuang, R.L.

Published
2020
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7. Joint analysis of energy and RMS spectra from MAXI J1535-571 with Insight-HXMT

Author

Kong, L.D., Zhang, S., Chen, Y.P., Ji, L., Zhang, S.N., Yang, Y.R., Tao, L., Ma, X., Qu, J.L., Lu, F.J., Bu, Q.C., Chen, L., Song, L.M., Li, T.P., Xu, Y.P., Cao, X.L., Chen, Y., Liu, C.Z., Cai, C., Chang, Z., Chen, G., Chen, T.X., Chen, Y.B., Cui, W., Cui, W.W., Deng, J.K., Dong, Y.W., Du, Y.Y., Fu, M.X., Gao, G.H., Gao, H., Gao, M., Ge, M.Y., Gu, Y.D., Guan, J., Guo, C.C., Han, D.W., Huang, Y., Huo, J., Jia, S.M., Jiang, L.H., Jiang, W.C., Jin, J., Li, B., Li, C.K., Li, G., Li, M.S., Li, W., Li, X., Li, X.B., Li, X.F., Li, Y.G., Li, Z.W., Liang, X.H., Liao, J.Y., Liu, G.Q., Liu, H.X., Liu, H.W., Liu, S.Z., Liu, X.J., Liu, Y.N., Lu, B., Lu, X.F., Luo, Q., Luo, T., Meng, B., Nang, Y., Nie, J.Y., Ou, G., Ren, X.Q., Sai, N., Song, X.Y., Sun, L., Tan, Y., Tuo, Y.L., Wang, C., Wang, G.F., Wang, J., Wang, P.J., Wang, W.S., Wang, Y.S., Wen, X.Y., Wu, B.Y., Wu, B.B., Wu, M., Xiao, G.C., Xiao, S., Xiong, S.L., Xu, H., Yang, J.W., Yang, S., Yang, Y.J., Yi, Q.B., You, Y., Zhang, A.M., Zhang, C.M., Zhang, F., Zhang, H.M., Zhang, J., Zhang, P., Zhang, T., Zhang, W., Zhang, W.C., Zhang, W.Z., Zhang, Y., Zhang, Y.F., Zhang, Y.J., Zhang, Y.H., Zhang, Z., Zhang, Z.L., Zhao, H.S., Zhao, X.F., Zheng, S.J., Zheng, Y.G., Zhou, D.K., Zhou, J.F., Zhu, Y.X., and Zhu, Y.

Published
2020
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8. Diagnostic of the spectral properties of Aquila X-1 by Insight-HXMT snapshots during the early propeller phase

Author

Güngör, C., Ge, M.Y., Zhang, S., Santangelo, A., Zhang, S.N., Lu, F.J., Zhang, Y., Chen, Y.P., Tao, L., Yang, Y.J., Bu, Q.C., Cai, C., Cao, X.L., Chang, Z., Chen, G., Chen, L., Chen, T.X., Chen, Y., Chen, Y.B., Cui, W., Cui, W.W., Deng, J.K., Dong, Y.W., Du, Y.Y., Fu, M.X., Gao, G.H., Gao, H., Gao, M., Gu, Y.D., Guan, J., Guo, C.C., Han, D.W., Huang, Y., Huo, J., Ji, L., Jia, S.M., Jiang, L.H., Jiang, W.C., Jin, J., Kong, L.D., Li, B., Li, C.K., Li, G., Li, M.S., Li, T.P., Li, W., Li, X., Li, X.B., Li, X.F., Li, Y.G., Li, Z.W., Liang, X.H., Liao, J.Y., Liu, C.Z., Liu, G.Q., Liu, H.W., Liu, X.J., Liu, Y.N., Lu, B., Lu, X.F., Luo, T., Luo, Q., Ma, X., Meng, B., Nang, Y., Nie, J.Y., Ou, G., Sai, N., Song, L.M., Song, X.Y., Sun, L., Tan, Y., Tuo, Y.L., Wang, C., Wang, G.F., Wang, J., Wang, W.S., Wang, Y.S., Wen, X.Y., Wu, B.B., Wu, B.Y., Wu, M., Xiao, G.C., Xiao, S., Xiong, S.L., Xu, Y.P., Yang, J.W., Yang, S., Yi, Q.B., Yin, Q.Q., You, Y., Zhang, A.M., Zhang, C.M., Zhang, F., Zhang, H.M., Zhang, J., Zhang, T., Zhang, W., Zhang, W.C., Zhang, W.Z., Zhang, Y.F., Zhang, Y.J., Zhang, Z., Zhang, Z.L., Zhao, H.S., Zhao, X.F., Zheng, S.J., Zhou, D.K., Zhou, J.F., Zhu, Y., and Zhu, Y.X.

Published
2020
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9. Insight-HXMT study of the timing properties of Sco X-1

Author

Jia, S.M., Bu, Q.C., Qu, J.L., Lu, F.J., Zhang, S.N., Huang, Y., Ma, X., Tao, L., Xiao, G.C., Zhang, W., Chen, L., Song, L.M., Zhang, S., Li, T.P., Xu, Y.P., Cao, X.L., Chen, Y., Liu, C.Z., Cai, C., Chang, Z., Chen, G., Chen, T.X., Chen, Y.B., Chen, Y.P., Cui, W., Cui, W.W., Deng, J.K., Dong, Y.W., Du, Y.Y., Fu, M.X., Gao, G.H., Gao, H., Gao, M., Ge, M.Y., Gu, Y.D., Guan, J., Guo, C.C., Han, D.W., Huo, J., Jiang, L.H., Jiang, W.C., Jin, J., Jin, Y.J., Kong, L.D., Li, B., Li, C.K., Li, G., Li, M.S., Li, W., Li, X., Li, X.B., Li, X.F., Li, Y.G., Li, Z.W., Liang, X.H., Liao, J.Y., Liu, G.Q., Liu, H.W., Liu, X.J., Liu, Y.N., Lu, B., Lu, X.F., Luo, Q., Luo, T., Meng, B., Nang, Y., Nie, J.Y., Ou, G., Sai, N., Shang, R.C., Song, X.Y., Sun, L., Tan, Y., Tuo, Y.L., Wang, C., Wang, G.F., Wang, J., Wang, W.S., Wang, Y.S., Wen, X.Y., Wu, B.Y., Wu, B.B., Wu, M., Xiao, S., Xiong, S.L., Yang, J.W., Yang, S., Yang, Y.J., Yin, Q.Q., Yi, Q.B., You, Y., Zhang, A.M., Zhang, C.M., Zhang, F., Zhang, H.M., Zhang, J., Zhang, T., Zhang, W.C., Zhang, W.Z., Zhang, Y., Zhang, Y.F., Zhang, Y.J., Zhang, Z., Zhang, Z.L., Zhao, H.S., Zhao, X.F., Zheng, S.J., Zhou, D.K., Zhou, J.F., Zhu, Y.X., Zhu, Y., and Zhuang, R.L.

Published
2020
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10. Insight-HXMT observation on 4U 1608–52: Evolving spectral properties of a bright type-I X-ray burst

Author

Chen, Y.P., Zhang, S., Zhang, S.N., Ji, L., Kong, L.D., Santangelo, A., Qu, J.L., Lu, F.J., Li, T.P., Song, L.M., Xu, Y.P., Cao, X.L., Chen, Y., Liu, C.Z., Bu, Q.C., Cai, C., Chang, Z., Chen, G., Chen, L., Chen, T.X., Chen, Y.B., Cui, W., Cui, W.W., Deng, J.K., Dong, Y.W., Du, Y.Y., Fu, M.X., Gao, G.H., Gao, H., Gao, M., Ge, M.Y., Gu, Y.D., Guan, J., Guo, C.C., Han, D.W., Huang, Y., Huo, J., Jia, S.M., Jiang, L.H., Jiang, W.C., Jin, J., Li, B., Li, C.K., Li, G., Li, M.S., Li, W., Li, X., Li, X.B., Li, X.F., Li, Y.G., Li, Z.W., Liang, X.H., Liao, J.Y., Liu, G.Q., Liu, H.W., Liu, X.J., Liu, Y.N., Lu, B., Lu, X.F., Luo, Q., Luo, T., Ma, X., Meng, B., Nang, Y., Nie, J.Y., Ou, G., Ren, X.Q., Sai, N., Sun, L., Tan, Y., Tao, L., Tuo, Y.L., Wang, C., Wang, G.F., Wang, J., Wang, W.S., Wang, Y.S., Wen, X.Y., Wu, B.Y., Wu, B.B., Wu, M., Xiao, G.C., Xiao, S., Xiong, S.L., Yang, J.W., Yang, S., Yang, Y.J., Yi, Q.B., Yin, Q.Q., You, Y., Zhang, A.M., Zhang, C.L., Zhang, C.M., Zhang, F., Zhang, H.M., Zhang, J., Zhang, T., Zhang, W.C., Zhang, W., Zhang, W.Z., Zhang, Yi., Zhang, Y.F., Zhang, Y.J., Zhang, Y., Zhang, Z., Zhang, Z.L., Zhao, H.S., Zhao, X.F., Zheng, S.J., Zhou, D.K., Zhou, J.F., Zhu, Y., and Zhu, Y.X.

Published
2019
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12. Constant cyclotron line energy in Hercules X–1 - Joint Insight-HXMT and NuSTAR observations

Author

Xiao, G.C., Ji, L., Staubert, R., Ge, M.Y., Zhang, S., Zhang, S.N., Santangelo, A., Ducci, L., Liao, J.Y., Guo, C.C., Li, X.B., Zhang, W., Qu, J.L., Lu, F.J., Li, T.P., Song, L.M., Xu, Y.P., Bu, Q.C., Cai, C., Cao, X.L., Chang, Z., Chen, G., Chen, L., Chen, T.X., Chen, Y.B., Chen, Y., Chen, Y.P., Cui, W., Cui, W.W., Deng, J.K., Dong, Y.W., Du, Y.Y., Fu, M.X., Gao, G.H., Gao, H., Gao, M., Gu, Y.D., Guan, J., Gungor, C., Han, D.W., Huang, Y., Huo, J., Jia, S.M., Jiang, L.H., Jiang, W.C., Jin, J., Kong, L.D., Li, B., Li, C.K., Li, G., Li, M.S., Li, W., Li, X., Li, X.F., Li, Y.G., Li, Z.W., Liang, X.H., Liu, C.Z., Liu, G.Q., Liu, H.W., Liu, X.J., Liu, Y.N., Lu, B., Lu, X.F., Luo, Q., Luo, T., Ma, X., Meng, B., Nang, Y., Nie, J.Y., Ou, G., Sai, N., Song, S.X., Sun, L., Tan, Y., Tao, L., Tuo, Y.L., Wang, C., Wang, G.F., Wang, J., Wang, W.S., Wang, Y.S., Wen, X.Y., Wu, B.B., Wu, B.Y., Wu, M., Xiong, S.L., Yang, J.W., Yang, S., Yang, Y.J., Yin, Q.B., Yin, Q.Q., Zhang, A.M., Zhang, C.M., Zhang, F., Zhang, H.M., Zhang, J., Zhang, T., Zhang, W.C., Zhang, W.Z., Zhang, Y., Zhang, Y.F., Zhang, Y.J., Zhang, Z., Zhang, Z.L., Zhao, H.S., Zhao, X.F., Zheng, S.J., Zhou, J.F., Zhu, Y., and Zhu, Y.X.

Published
2019
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13. Identification of a non-thermal X-ray burst with the Galactic magnetar SGR J1935+2154 and a fast radio burst using Insight-HXMT

Author

Li, C.K., primary, Lin, Lin, additional, Xiong, S.L., additional, Ge, Mingyu, additional, Li, X.B., additional, Li, Tipei, additional, Lu, F.J., additional, Zhang, Shuang-Nan, additional, Tuo, Y.L., additional, Nang, Y., additional, Zhang, B., additional, Xiao, S., additional, Chen, Y., additional, Song, L.M., additional, Xu, Y.P., additional, Liu, C.Z., additional, Jia, S.M., additional, Cao, X.L., additional, Qu, J.L., additional, Zhang, Shu, additional, Gu, Y.D., additional, Liao, J.Y., additional, Zhao, X.F., additional, Tan, Y., additional, Nie, J.Y., additional, Zhao, H.S., additional, Zheng, S.J., additional, Zheng, Y.G., additional, Luo, Qi, additional, Cai, C., additional, Li, B., additional, Xue, W.C., additional, Bu, Qingcui, additional, Chang, Zhi, additional, Chen, G., additional, Chen, T.X., additional, Chen, Yu-Peng, additional, Dong, Yong-Wei, additional, Du, Y.Y., additional, Gao, H., additional, Gao, G.H., additional, Gao, M., additional, Huo, J., additional, Han, D.W., additional, Jiang, L.H., additional, Huang, Y., additional, Jiang, Weichun, additional, Jin, J., additional, Kong, L.D., additional, Li, Gang, additional, Guan, J., additional, Li, M.S., additional, Li, W., additional, Li, X., additional, Li, X.F., additional, Li, Y.G., additional, Li, Z.W., additional, Liang, X.H., additional, Liu, B.S., additional, Liu, H.W., additional, Liu, X.J., additional, Lu, B., additional, Lu, X.F., additional, Luo, T., additional, Ma, X., additional, Meng, B., additional, Ou, G., additional, Sai, N., additional, Song, X.Y., additional, Sun, L., additional, Tao, Lian, additional, Wang, J., additional, Wang, G.F., additional, Wang, W.S., additional, Wang, Y.S., additional, Wen, X.Y., additional, Wu, B.B., additional, Wu, B.Y., additional, Wu, M., additional, Xiao, G.C., additional, Xu, H., additional, Yang, J.W., additional, Yang, S., additional, Yang, Yi-Jung, additional, Yang, Y.J., additional, Yi, Q.B., additional, Yin, Q.Q., additional, You, Y., additional, Zhang, C.M., additional, Zhang, A.M., additional, Zhang, F., additional, Zhang, H.M., additional, Zhang, J., additional, Zhang, T., additional, Zhang, Wei, additional, Zhang, W.C., additional, Zhang, Y., additional, Zhang, Yue, additional, Zhang, Y.F., additional, Zhang, Y.J., additional, Zhang, Z.L., additional, Zhou, D.K., additional, Zhu, Y., additional, Zhu, Y.X., additional, Chen, L., additional, Zhang, W.Z., additional, Chen, Y.B., additional, Cui, W., additional, Deng, J.K., additional, Fu, M.X., additional, Jin, Y.J., additional, Liu, G.Q., additional, Liu, Y.N., additional, Shang, R.C., additional, Zhang, Zhao, additional, Zhang, Zhi, additional, Zhou, J.F., additional, Wang, C., additional, Guo, C.C., additional, and Zhuang, R.L., additional

Published
2020
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14. Accretion in strong field gravity with eXTP

Author

De Rosa, Alessandra, Uttley, P., Gou, L. J., Liu, Y., Bambi, C., Barret, Didier, Belloni, T., Berti, E., Bianchi, Stefano, Caiazzo, I., Casella, P., Feroci, M., Ferrari, V., Gualtieri, L., Heyl, J., Ingram, A., Karas, V., Lu, F.J., Luo, B., Matt, G., Motta, S., Neilsen, J., Pani, P., Santangelo, A., Shu, X. W., Wang, J. F., Wang, J. M., Xue, Y. Q., Xu, Y. P., Yuan, W. M., Yuan, Y. F., Zhang, S. N., Zhang, S., Agudo, Iván, Amati, L., Andersson, N., Baglio, C., Bakala, P., Baykal, A., Bhattacharyya, S., Bombaci, I., Bucciantini, N., Capitanio, F., Ciolfi, R., Cui, W. K., D'Ammando, F., Dauser, T., Del Santo, M., De Marco, B., Linares, M., Migliari, S., Miniutti, Giovanni, Polish Academy of Sciences, Istituto Nazionale di Astrofisica, and Chinese Academy of Sciences

Subjects
X-ray, Accretion, Astrophysics::High Energy Astrophysical Phenomena, Black holes physics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract

In this paper we describe the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to accretion flows in the strong field gravity regime around both stellar-mass and supermassive black-holes. eXTP has the unique capability of using advanced “spectral-timing-polarimetry” techniques to analyze the rapid variations with three orthogonal diagnostics of the flow and its geometry, yielding unprecedented insight into the inner accreting regions, the effects of strong field gravity on the material within them and the powerful outflows which are driven by the accretion process. X-spinmeasurements.© 2018, Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature., The Italian collaboration acknowledged financial contribution from the agreement ASI-INAF n.2017-14-H.O. The Chinese team acknowledged the support of the Chinese Academy of Sciences through the Strategic Priority Research Program of the Chinese Academy of Sciences (Grant No. XDA15020100). A. Zdziarski acknowledges the Polish National Science Centre (Grant No. 2013/10/M/ST9/00729).

Published
2019

15. Accretion in strong field gravity with eXTP

Author

Polish Academy of Sciences, Istituto Nazionale di Astrofisica, Chinese Academy of Sciences, De Rosa, Alessandra, Uttley, P., Gou, L. J., Liu, Y., Bambi, C., Barret, Didier, Belloni, T., Berti, E., Bianchi, Stefano, Caiazzo, I., Casella, P., Feroci, M., Ferrari, V., Gualtieri, L., Heyl, J., Ingram, A., Karas, V., Lu, F.J., Luo, B., Matt, G., Motta, S., Neilsen, J., Pani, P., Santangelo, Andrea, Shu, X. W., Wang, J. F., Wang, J. M., Xue, Y. Q., Xu, Y. P., Yuan, W. M., Yuan, Y. F., Zhang, S. N., Zhang, S., Agudo, Iván, Amati, L., Andersson, N., Baglio, C., Bakala, P., Baykal, A., Bhattacharyya, S., Bombaci, I., Bucciantini, N., Capitanio, F., Ciolfi, Riccardo, Cui, W. K., D'Ammando, F., Dauser, T., Del Santo, M., De Marco, B., Linares, Manuel, Migliari, S., Miniutti, Giovanni, Polish Academy of Sciences, Istituto Nazionale di Astrofisica, Chinese Academy of Sciences, De Rosa, Alessandra, Uttley, P., Gou, L. J., Liu, Y., Bambi, C., Barret, Didier, Belloni, T., Berti, E., Bianchi, Stefano, Caiazzo, I., Casella, P., Feroci, M., Ferrari, V., Gualtieri, L., Heyl, J., Ingram, A., Karas, V., Lu, F.J., Luo, B., Matt, G., Motta, S., Neilsen, J., Pani, P., Santangelo, Andrea, Shu, X. W., Wang, J. F., Wang, J. M., Xue, Y. Q., Xu, Y. P., Yuan, W. M., Yuan, Y. F., Zhang, S. N., Zhang, S., Agudo, Iván, Amati, L., Andersson, N., Baglio, C., Bakala, P., Baykal, A., Bhattacharyya, S., Bombaci, I., Bucciantini, N., Capitanio, F., Ciolfi, Riccardo, Cui, W. K., D'Ammando, F., Dauser, T., Del Santo, M., De Marco, B., Linares, Manuel, Migliari, S., and Miniutti, Giovanni

Abstract

In this paper we describe the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to accretion flows in the strong field gravity regime around both stellar-mass and supermassive black-holes. eXTP has the unique capability of using advanced “spectral-timing-polarimetry” techniques to analyze the rapid variations with three orthogonal diagnostics of the flow and its geometry, yielding unprecedented insight into the inner accreting regions, the effects of strong field gravity on the material within them and the powerful outflows which are driven by the accretion process. X-spinmeasurements.© 2018, Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature.

Published
2019

18. eXTP: enhanced X-ray Timing and Polarimetry Mission

Author

den Herder, Jan-Willem A., Takahashi, Tadayuki, Bautz, Marshall, Zhang, S.N., Feroci, M., Santangelo, A., Dong, Y.W., Feng, H., Lu, F.J., Nandra, K., Wang, Z.S., Zhang, S., Bozzo, E., Brandt, Søren, Budtz-Jørgensen, Carl, Lund, Niels, den Herder, Jan-Willem A., Takahashi, Tadayuki, Bautz, Marshall, Zhang, S.N., Feroci, M., Santangelo, A., Dong, Y.W., Feng, H., Lu, F.J., Nandra, K., Wang, Z.S., Zhang, S., Bozzo, E., Brandt, Søren, Budtz-Jørgensen, Carl, and Lund, Niels

Published
2016

21. Ethmoid sinus mycology of chronic rhinosinusitis.

Author

Jiang, R.S., Liang, K.L., Shiao, J.Y., Lin, J.F., Su, M.C., Hsin, C.H., and Lu, F.J.

Subjects
MYCOLOGY, SINUSITIS, FUNGI, FUNGAL cultures, MUCOUS membranes, DNA
Abstract

This goal of this study was to demonstrate whether fungi were present in the ethmoid sinus in patients with chronic rhinosinusitis. Before surgery, swab specimens were collected from the middle meatus for conventional fungal cultures, and lavaged fluid was collected from the nasal cavity for fungal cultures by Ponikau’s method. During surgery, tissue specimens were taken from the inferior turbinate and the anterior ethmoid sinus for conventional fungal cultures and detection of fungal DNA by polymerase chain reaction. The ethmoid sinus mucosa with coating mucus was also collected for fungal cultures by Ponikau’s method. Among 53 specimens, three middle meatal specimens and 27 lavaged specimens (50.9%) grew fungi. Inferior turbinal mucosa did not grow fungi, but three ethmoid sinus specimens grew fungi by the conventional fungal culture method and by Ponikau’s method. Alternaria DNA was detected in 42 inferior turbinal specimens (79.3%) and in 39 ethmoid sinus specimens (73.6%). Our study showed that although fungi were rarely cultured from the ethmoid sinus Alternaria DNA was detected in most of the ethmoid sinus mucosa. [ABSTRACT FROM AUTHOR]

Published
2008
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