Search

Your search keyword '"Xu, R X"' showing total 528 results
Start Over Author "Xu, R X"
528 results on '"Xu, R X"'

151. Recent developments of inverse Compton scattering model of pulsar radio emission

Author

Qiao, G. J., Xu, R. X., Liu, J. F., and Han, B. Zhang J. L.

Subjects
Astrophysics
Abstract

Many theoretical efforts were made to understand the core and conal emission identified from observations by Rankin (1983) and Lyne and Manchester (1988). One of them, named as inverse Compton scattering (ICS) model (Qiao & Lin 1998), has been proposed. It is found in the model that: there are central or `core' emission beam, and one or two hollow conical emission beams; the different emission components are emitted at different heights; owing to different radiation components emitted from different height, the observed emission beams can be shifted from each other due to retardation and aberration effects; the sizes of emission components change with frequencies. Recent developments of the model include: simulations of pulse profiles at different frequencies; studying the basic polarization properties of inverse Compton scattering in strong magnetic fields; computing the polarizations and spectrum of core and cones. A new classification system was also proposed. The main results calculated from the model are consistent with the observations., Comment: 4 pages, no figures, LaTeX

Published
1999

152. Are Pulsars Bare Strange Stars?

Author

Xu, R. X., J, G., Qiao, ., and Zhang, B.

Subjects
Astrophysics
Abstract

It is believed that pulsars are neutron stars or strange stars with crusts. However we suggest here that pulsars may be bare strange stars (i.e., strange stars without crust). Due to rapid rotation and strong emission, young strange stars produced in supernova explosions should be bare when they act as radio pulsars. Because of strong magnetic field, two polar-crusts would shield the polar caps of an accreting strange star. Such a suggestion can be checked by further observations., Comment: 2 pages, no figures, LaTeX, Contribution to IAU Colloquium 177: Pulsar Astronomy -- 2000 and Beyond

Published
1999

153. High-energy accelerators above pulsar polar caps

Author

Xu, R. X., Qiao, G. J ., and Zhang, B.

Subjects
Astrophysics
Abstract

Similar to the terrestrial collision accelerators of electron-antielectron, another kind of accelerator is above a positively or negatively charged pulsar polar cap. In the case of pulsars with magnetic axis parallel (anti-parallel) to rotational axis, relativistic antielectron (electron) with Lorentz factor about 10^6 hit the electrons in the polar caps. These scenarios are investigated both for pulsars being bare strange stars and for pulsars being neutron stars. Such a study may be valuable to differentiate neutron stars and bare strange stars observationally., Comment: 2 pages, no figures, LaTeX, Contribution to IAU Colloquium 177: Pulsar Astronomy -- 2000 and Beyond

Published
1999

154. GRB: A Signature of Phase Transition to QGP?

Author

Xu, R. X., Dai, Z. G., Hong, B. H., and Qiao, G. J.

Subjects
Astrophysics
Abstract

It is suggested that the inner energetic engine of Gamma ray burst (GRB) may be the result of the transition of normal hadron to quark-gluon plasma (QGP) in rapidly-rotating and spin-down newborn neutron star. When such a nascent neutron star slows down through dipole electromagnetic and quadruple gravitational radiation, the increasing center density may reach the QCD transition density, i.e., 5-10 nuclear density. Such kind of energy release from the phase transition would be responsible for GRB and its possible beaming effect. The relative dense gaseous environment of GRB location and the iron line observed in the X-ray afterglow support this idea. Some predictions in this model are given. keywords: Gamma-ray Bursts, Supernova, Quark-gluon plasma, Comment: 7 pages, no figures, LaTeX, presented in 1999 Pacific Rim Conference of Stellar Astrophysics in Hong Kong University

Published
1999

155. Electric Character of Strange Stars

Author

Xu, R. X. and Qiao, G. J.

Subjects
Astrophysics
Abstract

Using the Thomas-Fermi model, we investigated the electric characteristics of a static non-magnetized strange star without crust in this paper. The exact solutions of electron number density and electric field above the quark surface are obtained. These results are useful if we are concerned about physical processes near the quark matter surfaces of strange stars., Comment: 4 pages, 2 figures, LaTeX, Published in Chinese Physics Letters, Vol.16, p.778

Published
1999
Full Text
View/download PDF

156. PSR 0943+10: a bare strange star?

Author

Xu, R. X., J, G., Qiao, ., and Zhang, Bing

Subjects
Astrophysics
Abstract

Recent work by Rankin & Deshpande strongly suggests that there exist strong ``micro-storms'' rotating around the magnetic axis of the 1.1s pulsar PSR 0943+10. Such a feature hints that most probably the large-voltage vacuum gap proposed by Ruderman & Sutherland (RS) does exist in the pulsar polar cap. However, there are severe arguments against the formation of the RS-type gap in pulsars, since the binding energies of both the Fe ions and the electrons in a neutron star's surface layer is too small to prevent thermionic ejection of the particles from the surface. Here we propose that PSR 0943+10 (probably also most of the other ``drifting'' pulsars) might be bare strange stars rather than normal neutron stars, in which the ``binding energy'' at the surface is merely infinity either for the case of ``pulsar'' or ``anti-pulsar''. It is further proposed that identifying a drifting pulsar as an anti-pulsar is the key criterion to distinguish strange stars from neutron stars., Comment: 4 pages, no figures, LaTeX, accepted 1999 July 9 by ApJ Letters

Published
1999
Full Text
View/download PDF

158. Circular polarization in pulsar integrated profiles

Author

Han, J. L., Manchester, R. N., Xu, R. X., and Qiao, G. J.

Subjects
Astrophysics
Abstract

We present a systematic study of the circular polarization in pulsar integrated profiles, based on published polarization data. For core components, we find no significant correlation between the sense-change of circular polarization and the sense of linear position angle variation. Circular polarization is not restricted to core components and, in some cases, reversals of circular polarization sense are observed across the conal emission. In conal double profiles, the sense of circular polarization is found to be correlated with the sense of position-angle variation. Pulsars with a high degree of linear polarization often have one hand of circular polarization across the whole profile. For most pulsars, the sign of circular polarization is the same at 50-cm and 20-cm wavelength, and the degree of polarization is similar, albeit with a wide scatter. However, at least two cases of frequency-dependent sign reversals are known. This diverse behaviour may require more than one mechanism to generate circular polarization., Comment: Will apear in MNRAS. 15 pages, 9 figures. One big table. 1.6MB PS file: ftp://ftp.mpifr-bonn.mpg.de/user/jhan/PS/98HMXQ_MN.ps

Published
1998
Full Text
View/download PDF

159. Pulsar radio emission from thunderstorms and raindrops of particles in the magnetosphere

Author

Chen, X., Yan, Y., Han, J. L., Wang, C., Wang, P. F., Jing, W. C., Lee, K. J., Zhang, B., Xu, R. X., Wang, T., Yang, Z. L., Su, W. Q., Cai, N. N., Wang, W. Y., Qiao, G. J., Xu, J., and Zhou, D. J.

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), FOS: Physical sciences, Astrophysics - High Energy Astrophysical Phenomena
Abstract

Pulsars radiate radio signals when they rotate. However, some old pulsars often stop radiating for some periods. The underlying mechanism remains unknown, while the magnetosphere during nulling phases is hard to probe due to the absence of emission measurement. Here we report the detection and accurate polarization measurements of sporadic weak narrow dwarf pulses detected in the ordinary nulling state of pulsar B2111+46 via the Five-Hundred-Meter Aperture Spherical radio Telescope (FAST). Further analysis shows that their polarization angles follow the average polarization angle curve of normal pulses, suggesting no change of magnetic field structure in the emission region in the two emission states. Whereas radio emission of normal individual pulses is radiated by a thunderstorm of particles produced by copious discharges in regularly formed gaps, dwarf pulses are produced by one or a few raindrops of particles generated by pair production in a fragile gap of this near-death pulsar., Comment: 37 pages, 15 figures. Authors version. Great FAST pulsar data

Published
2023
Full Text
View/download PDF

165. Exploring the single-pulse behaviours of PSR J0628+0909 with FAST.

Author

Hsu, J A, Jiang, J C, Xu, H, Lee, K J, and Xu, R X

Subjects
FARADAY effect, PULSARS, RADIO telescopes
Abstract

More than 100 rotating radio transients (RRATs) have been discovered since 2006. However, it is unclear whether RRATs radiate in nulling states. PSR J0628+0909 has been classified as an RRAT. In this paper, we study the single pulses and integrated pulse profile of PSR J0628+0909 to check whether we can detect pulsed radio emission in the nulling states. We also aim to study the polarization of the RRAT and its relationship to the general pulsar population. We used the Five-hundred-meter Aperture Spherical radio Telescope (FAST) to observe PSR J0628+0909 in the frequency range from 1.0 to 1.5 GHz. We searched for strong single pulses and looked for pulsed emission in the RRAT nulling states. Polarization profiles, the single-pulse energy distribution, and waiting-time statistics were measured. The Faraday rotation measure and dispersion measure values are updated with the current observation. The single-pulse polarization behaviours show great diversity, similar to the case of pulsars. Based on the integrated pulse profile and single-pulse energy statistics, we argue that continuous pulsar-like emission exists in addition to the transient-like burst emission for PSR J0628+0909. We find that the pulse waiting time is not correlated with the pulse energy and conclude that the strong transient emission of RRAT is not generated by the energy store–release mechanism. [ABSTRACT FROM AUTHOR]

Published
2023
Full Text
View/download PDF

168. Observation of the Crab Nebula with LHAASO-KM2A − a performance study *

Author

Aharonian, F., primary, An, Q., additional, Axikegu, 克古, additional, Bai, L. X., additional, Bai, Y. X., additional, Bao, Y. W., additional, Bastieri, D., additional, Bi, X. J., additional, Bi, Y. J., additional, Cai, H., additional, Cai, J. T., additional, Cao, Z., additional, Chang, J., additional, Chang, J. F., additional, Chang, X. C., additional, Chen, B. M., additional, Chen, J., additional, Chen, L., additional, Chen, M. J., additional, Chen, M. L., additional, Chen, Q. H., additional, Chen, S. H., additional, Chen, S. Z., additional, Chen, T. L., additional, Chen, X. L., additional, Chen, Y., additional, Cheng, N., additional, Cheng, Y. D., additional, Cui, S. W., additional, Cui, X. H., additional, Cui, Y. D., additional, Dai, B. Z., additional, Dai, H. L., additional, Dai, Z. G., additional, Danzengluobu, 罗布, additional, Volpe, D. della, additional, Piazzoli, B. D'Ettorre, additional, Dong, X. J., additional, Fan, J. H., additional, Fan, Y. Z., additional, Fan, Z. X., additional, Fang, J., additional, Fang, K., additional, Feng, C. F., additional, Feng, L., additional, Feng, S. H., additional, Feng, Y. L., additional, Gao, B., additional, Gao, C. D., additional, Gao, Q., additional, Gao, W., additional, Ge, M. M., additional, Geng, L. S., additional, Gong, G. H., additional, Gou, Q. B., additional, Gu, M. H., additional, Guo, J. G., additional, Guo, X. L., additional, Guo, Y. Q., additional, Guo, Y. Y., additional, Han, Y. A., additional, He, H. H., additional, He, H. N., additional, He, J. C., additional, He, S. L., additional, He, X. B., additional, He, Y., additional, Heller, M., additional, Hor, Y. K., additional, Hou, C., additional, Hou, X., additional, Hu, H. B., additional, Hu, S., additional, Hu, S. C., additional, Hu, X. J., additional, Huang, D. H., additional, Huang, Q. L., additional, Huang, W. H., additional, Huang, X. T., additional, Huang, Z. C., additional, Ji, F., additional, Ji, X. L., additional, Jia, H. Y., additional, Jiang, K., additional, Jiang, Z. J., additional, Jin, C., additional, Kuleshov, D., additional, Levochkin, K., additional, Li, B. B., additional, Li, C., additional, Li, F., additional, Li, H. B., additional, Li, H. C., additional, Li, H. Y., additional, Li, J., additional, Li, K., additional, Li, W. L., additional, Li, X., additional, Li, X. R., additional, Li, Y., additional, Li, Y. Z., additional, Li, Z., additional, Liang, E. W., additional, Liang, Y. F., additional, Lin, S. J., additional, Liu, B., additional, Liu, C., additional, Liu, D., additional, Liu, H., additional, Liu, H. D., additional, Liu, J., additional, Liu, J. L., additional, Liu, J. S., additional, Liu, J. Y., additional, Liu, M. Y., additional, Liu, R. Y., additional, Liu, S. M., additional, Liu, W., additional, Liu, Y. N., additional, Liu, Z. X., additional, Long, W. J., additional, Lu, R., additional, Lv, H. K., additional, Ma, B. Q., additional, Ma, L. L., additional, Ma, X. H., additional, Mao, J. R., additional, Masood, A., additional, Mitthumsiri, W., additional, Montaruli, T., additional, Nan, Y. C., additional, Pang, B. Y., additional, Pattarakijwanich, P., additional, Pei, Z. Y., additional, Qi, M. Y., additional, Ruffolo, D., additional, Rulev, V., additional, Sáiz, A., additional, Shao, L., additional, Shchegolev, O., additional, Sheng, X. D., additional, Shi, J. R., additional, Song, H. C., additional, Stenkin, Yu. V., additional, Stepanov, V., additional, Sun, Q. N., additional, Sun, X. N., additional, Sun, Z. B., additional, Tam, P. H. T., additional, Tang, Z. B., additional, Tian, W. W., additional, Wang, B. D., additional, Wang, C., additional, Wang, H., additional, Wang, H. G., additional, Wang, J. C., additional, Wang, J. S., additional, Wang, L. P., additional, Wang, L. Y., additional, Wang, R. N., additional, Wang, W., additional, Wang, X. G., additional, Wang, X. J., additional, Wang, X. Y., additional, Wang, Y. D., additional, Wang, Y. J., additional, Wang, Y. P., additional, Wang, Z., additional, Wang, Z. H., additional, Wang, Z. X., additional, Wei, D. M., additional, Wei, J. J., additional, Wei, Y. J., additional, Wen, T., additional, Wu, C. Y., additional, Wu, H. R., additional, Wu, S., additional, Wu, W. X., additional, Wu, X. F., additional, Xi, S. Q., additional, Xia, J., additional, Xia, J. J., additional, Xiang, G. M., additional, Xiao, G., additional, Xiao, H. B., additional, Xin, G. G., additional, Xin, Y. L., additional, Xing, Y., additional, Xu, D. L., additional, Xu, R. X., additional, Xue, L., additional, Yan, D. H., additional, Yang, C. W., additional, Yang, F. F., additional, Yang, J. Y., additional, Yang, L. L., additional, Yang, M. J., additional, Yang, R. Z., additional, Yang, S. B., additional, Yao, Y. H., additional, Yao, Z. G., additional, Ye, Y. M., additional, Yin, L. Q., additional, Yin, N., additional, You, X. H., additional, You, Z. Y., additional, Yu, Y. H., additional, Yuan, Q., additional, Zeng, H. D., additional, Zeng, T. X., additional, Zeng, W., additional, Zeng, Z. K., additional, Zha, M., additional, Zhai, X. X., additional, Zhang, B. B., additional, Zhang, H. M., additional, Zhang, H. Y., additional, Zhang, J. L., additional, Zhang, J. W., additional, Zhang, L., additional, Zhang, L. X., additional, Zhang, P. F., additional, Zhang, P. P., additional, Zhang, R., additional, Zhang, S. R., additional, Zhang, S. S., additional, Zhang, X., additional, Zhang, X. P., additional, Zhang, Y., additional, Zhang, Y. F., additional, Zhang, Y. L., additional, Zhao, B., additional, Zhao, J., additional, Zhao, L., additional, Zhao, L. Z., additional, Zhao, S. P., additional, Zheng, F., additional, Zheng, Y., additional, Zhou, B., additional, Zhou, H., additional, Zhou, J. N., additional, Zhou, P., additional, Zhou, R., additional, Zhou, X. X., additional, Zhu, C. G., additional, Zhu, F. R., additional, Zhu, H., additional, Zhu, K. J., additional, and Zuo, X., additional

Published
2021
Full Text
View/download PDF

169. Residual cholesterol as prognostic predictor associates with different glucose metabolism status in patients with coronary artery disease

Author

Cao, Y.-X., primary, Zhang, H.-W., additional, Jin, J.-L., additional, Liu, H.-H., additional, Zhang, Y., additional, Xu, R.-X., additional, Gao, Y., additional, Guo, Y.-L., additional, Wu, N.-Q., additional, Zhu, C.-G., additional, Hua, Q., additional, Li, Y.-F., additional, Cui, C.-J., additional, Dong, Q., additional, Sun, J., additional, and Li, J.-J., additional

Published
2020
Full Text
View/download PDF

171. No pulsed radio emission during a bursting phase of a Galactic magnetar

Author

Lin, L., primary, Zhang, C. F., additional, Wang, P., additional, Gao, H., additional, Guan, X., additional, Han, J. L., additional, Jiang, J. C., additional, Jiang, P., additional, Lee, K. J., additional, Li, D., additional, Men, Y. P., additional, Miao, C. C., additional, Niu, C. H., additional, Niu, J. R., additional, Sun, C., additional, Wang, B. J., additional, Wang, Z. L., additional, Xu, H., additional, Xu, J. L., additional, Xu, J. W., additional, Yang, Y. H., additional, Yang, Y. P., additional, Yu, W., additional, Zhang, B., additional, Zhang, B.-B., additional, Zhou, D. J., additional, Zhu, W. W., additional, Castro-Tirado, A. J., additional, Dai, Z. G., additional, Ge, M. Y., additional, Hu, Y. D., additional, Li, C. K., additional, Li, Y., additional, Li, Z., additional, Liang, E. W., additional, Jia, S. M., additional, Querel, R., additional, Shao, L., additional, Wang, F. Y., additional, Wang, X. G., additional, Wu, X. F., additional, Xiong, S. L., additional, Xu, R. X., additional, Yang, Y.-S., additional, Zhang, G. Q., additional, Zhang, S. N., additional, Zheng, T. C., additional, and Zou, J.-H., additional

Published
2020
Full Text
View/download PDF

172. Diverse polarization angle swings from a repeating fast radio burst source

Author

Luo, R., primary, Wang, B. J., additional, Men, Y. P., additional, Zhang, C. F., additional, Jiang, J. C., additional, Xu, H., additional, Wang, W. Y., additional, Lee, K. J., additional, Han, J. L., additional, Zhang, B., additional, Caballero, R. N., additional, Chen, M. Z., additional, Chen, X. L., additional, Gan, H. Q., additional, Guo, Y. J., additional, Hao, L. F., additional, Huang, Y. X., additional, Jiang, P., additional, Li, H., additional, Li, J., additional, Li, Z. X., additional, Luo, J. T., additional, Pan, J., additional, Pei, X., additional, Qian, L., additional, Sun, J. H., additional, Wang, M., additional, Wang, N., additional, Wen, Z. G., additional, Xu, R. X., additional, Xu, Y. H., additional, Yan, J., additional, Yan, W. M., additional, Yu, D. J., additional, Yuan, J. P., additional, Zhang, S. B., additional, and Zhu, Y., additional

Published
2020
Full Text
View/download PDF

176. An in-depth investigation of 11 pulsars discovered by FAST

Author

Cameron, A D, primary, Li, D, primary, Hobbs, G, primary, Zhang, L, primary, Miao, C C, primary, Wang, J B, primary, Yuan, M, primary, Wang, S, primary, Jacobs Corban, G, primary, Cruces, M, primary, Dai, S, primary, Feng, Y, primary, Han, J, primary, Kaczmarek, J F, primary, Niu, J R, primary, Pan, Z C, primary, Qian, L, primary, Tao, Z Z, primary, Wang, P, primary, Wang, S Q, primary, Xu, H, primary, Xu, R X, primary, Yue, Y L, primary, Zhang, S B, primary, Zhi, Q J, primary, Zhu, W W, primary, Champion, D J, primary, Kramer, M, primary, Zhou, S Q, primary, Qiu, K P, primary, and Zhu, M, primary

Published
2020
Full Text
View/download PDF

181. Piggyback search for fast radio bursts using Nanshan 26 m and Kunming 40 m radio telescopes – I. Observing and data analysis systems, discovery of a mysterious peryton

Author

Men, Y P, primary, Luo, R, additional, Chen, M Z, additional, Hao, L F, additional, Lee, K J, additional, Li, J, additional, Li, Z X, additional, Liu, Z Y, additional, Pei, X, additional, Wen, Z G, additional, Wu, J J, additional, Xu, Y H, additional, Xu, R X, additional, Yuan, J P, additional, and Zhang, C F, additional

Published
2019
Full Text
View/download PDF

183. Non-Markovian response of ultrafast coherent electronic ring currents in chiral aromatic molecules in a condensed phase.

Author

Mineo, H., Lin, S. H., Fujimura, Y., Xu, J., Xu, R. X., and Yan, Y. J.

Subjects
MARKOV spectrum, COHERENCE (Physics), ELECTRIC currents, CHIRALITY, AROMATIC compounds, CONDENSED matter, FEMTOSECOND lasers
Abstract

Results of a theoretical study on non-Markov response for femtosecond laser-driven coherent ring currents in chiral aromatic molecules embedded in a condensed phase are presented. Coherent ring currents are generated by coherent excitation of a pair of quasi-degenerated π-electronic excited states. The coherent electronic dynamical behaviors are strongly influenced by interactions between the electronic system and phonon bath in a condensed phase. Here, the bath correlation time is not instantaneous but should be taken to be a finite time in ultrashort time-resolved experiments. In such a case, Markov approximation breaks down. A hierarchical master equation approach for an improved semiclassical Drude dissipation model was adopted to examine the non-Markov effects on ultrafast coherent electronic ring currents of (P)-2,2′-biphenol in a condensed phase. Time evolution of the coherent ring current derived in the hierarchical master equation approach was calculated and compared with those in the Drude model in the Markov approximation and in the static limit. The results show how non-Markovian behaviors in quantum beat signals of ring currents depend on the Drude bath damping constant. Effects of temperatures on ultrafast coherent electronic ring currents are also clarified. [ABSTRACT FROM AUTHOR]

Published
2013
Full Text
View/download PDF

187. eXTP: Enhanced X-ray Timing and Polarization mission

Author

Zhang, S. N., additional, Feroci, M., additional, Santangelo, A., additional, Dong, Y. W., additional, Feng, H., additional, Lu, F. J., additional, Nandra, K., additional, Wang, Z. S., additional, Zhang, S., additional, Bozzo, E., additional, Brandt, S., additional, De Rosa, A., additional, Gou, L. J., additional, Hernanz, M., additional, van der Klis, M., additional, Li, X. D., additional, Liu, Y., additional, Orleanski, P., additional, Pareschi, G., additional, Pohl, M., additional, Poutanen, J., additional, Qu, J. L., additional, Schanne, S., additional, Stella, L., additional, Uttley, P., additional, Watts, A., additional, Xu, R. X., additional, Yu, W. F., additional, in ’t Zand, J. J. M., additional, Zane, S., additional, Alvarez, L., additional, Amati, L., additional, Baldini, L., additional, Bambi, C., additional, Basso, S., additional, Bhattacharyya, S., additional, Bellazzini, R., additional, Belloni, T., additional, Bellutti, P., additional, Bianchi, S., additional, Brez, A., additional, Bursa, M., additional, Burwitz, V., additional, Budtz-Jørgensen, C., additional, Caiazzo, I., additional, Campana, R., additional, Cao, X. L., additional, Casella, P., additional, Chen, C. Y., additional, Chen, L., additional, Chen, T., additional, Chen, Y., additional, Chen, Y. P., additional, Civitani, M., additional, Coti Zelati, F., additional, Cui, W., additional, Cui, W. W., additional, Dai, Z. G., additional, Del Monte, E., additional, de Martino, D., additional, Di Cosimo, S., additional, Diebold, S., additional, Dovciak, M., additional, Donnarumma, I., additional, Doroshenko, V., additional, Esposito, P., additional, Evangelista, Y., additional, Favre, Y., additional, Friedrich, P., additional, Fuschino, F., additional, Galvez, J. L., additional, Gao, Z. L., additional, Ge, M. Y., additional, Gevin, O., additional, Goetz, D., additional, Han, D. W., additional, Heyl, J., additional, Horak, J., additional, Hu, W., additional, Huang, F., additional, Huang, Q. S., additional, Hudec, R., additional, Huppenkothen, D., additional, Israel, G. L., additional, Ingram, A., additional, Karas, V., additional, Karelin, D., additional, Jenke, P. A., additional, Ji, L., additional, Korpela, S., additional, Kunneriath, D., additional, Labanti, C., additional, Li, G., additional, Li, X., additional, Li, Z. S., additional, Liang, E. W., additional, Limousin, O., additional, Lin, L., additional, Ling, Z. X., additional, Liu, H. B., additional, Liu, H. W., additional, Liu, Z., additional, Lu, B., additional, Lund, N., additional, Lai, D., additional, Luo, B., additional, Luo, T., additional, Ma, B., additional, Mahmoodifar, S., additional, Marisaldi, M., additional, Martindale, A., additional, Meidinger, N., additional, Men, Y. P., additional, Michalska, M., additional, Mignani, R., additional, Minuti, M., additional, Motta, S., additional, Muleri, F., additional, Neilsen, J., additional, Orlandini, M., additional, Pan, A. T., additional, Patruno, A., additional, Perinati, E., additional, Picciotto, A., additional, Piemonte, C., additional, Pinchera, M., additional, Rachevski, A., additional, Rapisarda, M., additional, Rea, N., additional, Rossi, E. M. R., additional, Rubini, A., additional, Sala, G., additional, Shu, X. W., additional, Sgro, C., additional, Shen, Z. X., additional, Soffitta, P., additional, Song, L. M., additional, Spandre, G., additional, Stratta, G., additional, Strohmayer, T. E., additional, Sun, L., additional, Svoboda, J., additional, Tagliaferri, G., additional, Tenzer, C., additional, Hong, T., additional, Taverna, R., additional, Torok, G., additional, Turolla, R., additional, Vacchi, S., additional, Wang, J., additional, Walton, D., additional, Wang, K., additional, Wang, J. F., additional, Wang, R. J., additional, Wang, Y. F., additional, Weng, S. S., additional, Wilms, J., additional, Winter, B., additional, Wu, X., additional, Wu, X. F., additional, Xiong, S. L., additional, Xu, Y. P., additional, Xue, Y. Q., additional, Yan, Z., additional, Yang, S., additional, Yang, X., additional, Yang, Y. J., additional, Yuan, F., additional, Yuan, W. M., additional, Yuan, Y. F., additional, Zampa, G., additional, Zampa, N., additional, Zdziarski, A., additional, Zhang, C., additional, Zhang, C. L., additional, Zhang, L., additional, Zhang, X., additional, Zhang, Z., additional, Zhang, W. D., additional, Zheng, S. J., additional, Zhou, P., additional, and Zhou, X. L., additional

Published
2016
Full Text
View/download PDF

190. A study of multifrequency polarization pulse profiles of millisecond pulsars

Author

Dai, S., primary, Hobbs, G., additional, Manchester, R. N., additional, Kerr, M., additional, Shannon, R. M., additional, van Straten, W., additional, Mata, A., additional, Bailes, M., additional, Bhat, N. D. R., additional, Burke-Spolaor, S., additional, Coles, W. A., additional, Johnston, S., additional, Keith, M. J., additional, Levin, Y., additional, Osłowski, S., additional, Reardon, D., additional, Ravi, V., additional, Sarkissian, J. M., additional, Tiburzi, C., additional, Toomey, L., additional, Wang, H. G., additional, Wang, J.-B., additional, Wen, L., additional, Xu, R. X., additional, Yan, W. M., additional, and Zhu, X.-J., additional

Published
2015
Full Text
View/download PDF

Catalog

Books, media, physical & digital resources
See catalog results