Relevant bibliographies by topics / X-­ray pulsars

Contents

  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'X-­ray pulsars'

Author: Grafiati
Published: 6 September 2023
Last updated: 25 July 2025

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Journal articles on the topic "X-­ray pulsars"

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Zhang, Xinyuan, Ping Shuai, Liangwei Huang, Shaolong Chen, and Lihong Xu. "Mission Overview and Initial Observation Results of the X-Ray Pulsar Navigation-I Satellite." International Journal of Aerospace Engineering 2017 (2017): 1–7. http://dx.doi.org/10.1155/2017/8561830.

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The newly launched X-ray pulsar navigation-I (XPNAV-1) is an experimental satellite of China that is designed for X-ray pulsar observation. This paper presents the initial observation results and aims to recover the Crab pulsar’s pulse profile to verify the X-ray instrument’s capability of observing pulsars in space. With the grazing-incidence focusing type instrument working at the soft X-ray band (0.5–10 keV), up to 162 segments of observations of the Crab pulsar are fulfilled, and more than 5 million X-ray events are recorded. Arrival times of photons are corrected to the solar system baryc
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Kawai, Nobuyuki, and Keisuke Tamura. "Recent X-ray Observations of Pulsar Nebulae." International Astronomical Union Colloquium 160 (1996): 367–74. http://dx.doi.org/10.1017/s0252921100041920.

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AbstractResults from the X-ray observations of pulsars with ASCA are presented. The surroundings of pulsars are investigated in detail taking advantage of ASCA’s unique capabilities; high spectral resolution and a high throughput over a wide energy range from 0.4 keV to 10 keV. The spectral characteristics of the nebulae of PSR B1509—58 and the Vela pulsar are spectroscopically investigated. A jet-like feature is found from PSR B1509—58. We detected diffuse emission sources in the vicinity of many pulsars. The high probability of finding such diffuse sources for many pulsars suggests that they
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Liang, Hao, Yafeng Zhan, and Chaowei Duan. "A Bayesian Classifier for X-Ray Pulsars Recognition." International Journal of Aerospace Engineering 2016 (2016): 1–10. http://dx.doi.org/10.1155/2016/1746925.

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Recognition for X-ray pulsars is important for the problem of spacecraft’s attitude determination by X-ray Pulsar Navigation (XPNAV). By using the nonhomogeneous Poisson model of the received photons and the minimum recognition error criterion, a classifier based on the Bayesian theorem is proposed. For X-ray pulsars recognition with unknown Doppler frequency and initial phase, the features of every X-ray pulsar are extracted and the unknown parameters are estimated using the Maximum Likelihood (ML) method. Besides that, a method to recognize unknown X-ray pulsars or X-ray disturbances is prop
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Wang, H. G., G. J. Qiao, and R. X. Xu. "Phase Offset of Rotation-Powered X-ray Pulsars." Symposium - International Astronomical Union 214 (2003): 224–26. http://dx.doi.org/10.1017/s0074180900194458.

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Combing the data of all the 10 rotation-powered pulsars that have measurements of relative phase of radio and X-ray pulses, we report here the behavior of radio/X-ray phase offset. We find that the radio/X-ray offset of normal pulsars does not show the trend of increase with increasing pulsar period as the radio/gamma-ray offset exhibits. The offset of millisecond pulsars is generally much less than that of the normal pulsars. Such phenomenon should also be taken into account by the high energy models for pulsars.
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ANKAY, AŞKIN, SERKAN ŞAHIN, GÖKÇE KARANFIL, and EFE YAZGAN. "EARLY PHASES OF DIFFERENT TYPES OF ISOLATED NEUTRON STAR." International Journal of Modern Physics D 14, no. 06 (2005): 1075–82. http://dx.doi.org/10.1142/s0218271805006535.

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Two Galactic isolated strong X-ray pulsars seem to be in the densest environments compared to other types of Galactic pulsar. X-ray pulsar J1846-0258 can be in an early phase of anomalous X-ray pulsars and soft gamma repeaters if its average braking index is ~1.8–2.0. X-ray pulsar J1811-1925 must have a very large average braking index (~11) if this pulsar was formed by SN 386AD. This X-ray pulsar can be in an early phase of the evolution of the radio pulsars located in the region P ~ 50–150 ms and Ṗ ~ 10-14–10-16 ss -1 of the P–Ṗ diagram. X-ray/radio pulsar J0540-69 seems to be evolving in th
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Becker, W. "X-ray Emission Characteristics of Pulsars." Symposium - International Astronomical Union 195 (2000): 49–60. http://dx.doi.org/10.1017/s0074180900162771.

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Recent X-ray observatories such as ROSAT, ASCA, RXTE, BeppoSAX, and Chandra have achieved important progress in neutron star and pulsar astronomy. The identification of Geminga as a rotation-powered pulsar, the discovery of X-ray emission from millisecond pulsars, and the identification of cooling neutron stars are only a few of the fascinating results. In the following, I will give a brief review on the X-ray emission properties of rotation-powered pulsars and their wind nebulae.
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Pivovaroff, M. J., V. M. Kaspi, and F. Camilo. "X-ray observations of the high magnetic field radio pulsar PSR J1814–1744." International Astronomical Union Colloquium 177 (2000): 349–50. http://dx.doi.org/10.1017/s0252921100059959.

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AbstractWe present X-ray observations of PSR J1814–1744, a 4 s radio pulsar with inferred surface dipole magnetic field strength 5.5 × 1013G recently discovered in the on-going Parkes multibeam survey. This pulsar’s spin parameters are very similar to those of anomalous X-ray pulsars (AXPs). X-ray emission is not detected from the position of the radio pulsar in observations withROSATandASCA. The derived upper flux limit implies an X-ray luminosity significantly smaller than those of all known AXPs. These results argue that magnetar mechanism invoked to explain X-ray emission from AXPs must de
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Kawai, N., Keisuke Tamura, and S. Shibata. "New Detection of X-Ray Pulsar Nebulae by ASCA." Symposium - International Astronomical Union 188 (1998): 265–66. http://dx.doi.org/10.1017/s0074180900115062.

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X-ray images of rotation-powered pulsars were examined using ASCA Gas Imaging Spectrometer (GIS). The data sets are taken from those available in the ASCA public archive in the performance verification (PV) phase and the guest-observing (GO) phase 1. We detected diffuse X-ray sources in the vicinity of nine pulsars including five new detections. There are large variety in their morphology and spatial size. The high probability of finding such diffuse sources around pulsars suggests that they exist universally for all the active pulsars, and that they are powered by the pulsars. We propose that
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Pivovaroff, M. J., V. M. Kaspi, and E. V. Gotthelf. "ASCA observations of Galactic rotation-powered pulsars." International Astronomical Union Colloquium 177 (2000): 351–52. http://dx.doi.org/10.1017/s0252921100059960.

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AbstractWe have examined several archivalASCAobservations of Galactic radio pulsars, including PSRs B1046–58 and B1610–50. X-ray emission is detected from PSR B1046–58 with a significance of ∼5σ. We find no evidence for pulsations. We argue that the emission is from a spatially unresolved synchrotron nebula powered by the pulsar. The location of the X-ray counterpart within the 95% position error ellipse of the gamma-ray source 3EG J1048–5840 strengthens the claim of Kaspi et al. (2000) that PSR B1046–58 emitϒ-rays. X-ray emission from PSR B1610–50 is not detected. We use the X-ray luminosity
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Aoki, Yu, Takahiro Enomoto, Yoichi Yatsu, et al. "Searching for X-ray counterparts of Fermi Gamma-ray pulsars in Suzaku observations." Proceedings of the International Astronomical Union 7, S279 (2011): 317–18. http://dx.doi.org/10.1017/s1743921312013130.

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AbstractWe report the Suzaku follow-up observations of the Gamma-ray pulsars, 1FGL J0614,13328, J1044.55737, J1741.82101, and J1813.31246, which were discovered by the Fermi Gamma-ray observatory. Analysing Suzaku/XIS data, we detected X-ray counterparts of these pulsars in the Fermi error circle and interpreted their spectra with absorbed power-law functions. These results indicate that the origin of these X-ray sources is non-thermal emission from the pulsars or from Pulsar Wind Nebulae (PWNe) surrounding them. Moreover we found that J1741.82101 exhibits a peculiar profile: spin-down luminos
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Dissertations / Theses on the topic "X-­ray pulsars"

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Gavriil, Fotis Panagiotis. "Magnetar-like x-ray bursts from anomalous x-ray pulsars." Thesis, McGill University, 2006. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=100371.

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The leading model for understanding the energetics of anomalous X-ray pulsars (AXPs) is that they are "magnetars"---young, isolated neutron stars powered by the decay of their enormous magnetic fields. The identification of AXPs as magnetars is motivated by the similarity of AXPs to another enigmatic class of sources, the Soft Gamma Repeaters (SGRs). We report on long-term monitoring of AXPs using the Rossi X-ray Timing Explorer (RXTE). We monitor AXPs with RXTE to study their rotational stability, to search for variations in their pulsed flux and pulsed morphology. During our regular monitori
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Tang, Pui-shan Anisia, and 鄧佩姗. "Thermal X-ray pulses resulting from pulsar glitches." Thesis, The University of Hong Kong (Pokfulam, Hong Kong), 1999. http://hub.hku.hk/bib/B29790992.

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Tang, Pui-shan Anisia. "Thermal X-ray pulses resulting from pulsar glitches /." Hong Kong : University of Hong Kong, 1999. http://sunzi.lib.hku.hk/hkuto/record.jsp?B2089675X.

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Inam, Sitki Cagdas. "X-ray Observations Of Accretion Powered Pulsars." Phd thesis, METU, 2004. http://etd.lib.metu.edu.tr/upload/12605552/index.pdf.

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In this thesis, X-ray observations of four accretion powered pulsars are presented. Using RXTE observations of 4U 1907+09, we found three new pulse periods of the source. We found that the source spun-down almost at a constant rate of $dot nu$ = (-3.54 $pm 0.02) times 10^{-14}$ Hz s$^{-1}$ for more than 15 years. Using RXTE observations, X-ray flux related spectral and timing features in 2S 1417-62 were, in general, interpreted as a sign of a disc accretion with a similar geometry with a varying mass accretion rate, whereas spectral and timing features of the low X-ray flux regions were
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吳國偉 and Kwok-wai Eddie Ng. "Neutrino production from accreting X-ray pulsars." Thesis, The University of Hong Kong (Pokfulam, Hong Kong), 1993. http://hub.hku.hk/bib/B31211811.

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Ng, Kwok-wai Eddie. "Neutrino production from accreting X-ray pulsars /." [Hong Kong : University of Hong Kong], 1993. http://sunzi.lib.hku.hk/hkuto/record.jsp?B13745013.

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Icdem, Burcin. "Viscous Time Scale In Accreting Powered Pulsars And Anomalous X-ray Pulsars." Master's thesis, METU, 2011. http://etd.lib.metu.edu.tr/upload/12613373/index.pdf.

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In this thesis we analyse X-ray data of accretion powered low mass and high mass X-ray binaries to understand the nature of their accretion mechanisms by searching for some clues of viscous time-scales of their accretion discs, if they have, in their low frequency power density spectra created from their long-term X-ray observations, or by doing pulse timing analysis with much shorter X-ray data to detect the effects of torque fluctuations caused by the accreting material on the pulsar. The low mass and high mass X-ray binaries we analysed have breaks in their power density spectra, which are
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Dib, Rim. "RXTE monitoring of 5 anomalous x-ray pulsars." Thesis, McGill University, 2009. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=66730.

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Anomalous X-ray Pulsars (AXPs) are a group of neutron stars that share several common properties. They are dubbed "anomalous'' because their observed luminosity exceeds the rate of loss of their rotational kinetic energy. According to the magnetar model, they are young, isolated neutron stars, powered by a large magnetic energy reservoir. Five of these AXPs (1E 2259+586, 4U 0142+61, RXS J170849.0-400910, 1E 1841-045, 1E 1048.1-5937) have been monitored with the Rossi X-ray Timing Explorer (RXTE) since 1997 (1998 for two of the sources). The goal of the monitoring program is to stud
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Camero, Arranz Ascension. "Accreting X-Ray pulsars. The high energy picture." Doctoral thesis, Universitat de València, 2007. http://hdl.handle.net/10803/9484.

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El objetivo principal de esta tesis ha sido el estudio del comportamiento transitorio durante estallidos de distinto tipo, de una selección de pulsares acretores en rayos X, localizados en el plano galáctico.Con ello se pretende haber avanzado hacia una explicación más clara de la naturaleza de estas objetos binarios de alta masa (con estrella de neutrones como objeto compacto), así como de los mecanismos físicos que operan en este escenario. Para todo esto se han analizado datos de dos misiones espaciales:INTEGRA Y RXTE.El segundo objetivo ha sido el estudio de la zona del brazo galactico de
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Gavriil, Fotis P. "Long-term monitoring of anomalous X-ray pulsars with the rossi x-ray timing explorer." Thesis, McGill University, 2001. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=33763.

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We report on the long-term monitoring of five anomalous X-ray Pulsars (AXPs) using the Rossi X-ray Timing Explorer (RXTE ). We present a phase-coherent timing ephemeris for 4U 0142+61, and show that it has rotated with high stability over 4.4 yr, with RMS phase deviation of 7% of the pulse period from a simple fit including only n and n&d2; . We show that 1E 1048.1-5937 shows significant deviations from simple spin-down such that phase-coherent timing has not been possible over time spans longer than a few months. We find that the deviations from simple spin down are not consistent with single
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Books on the topic "X-­ray pulsars"

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NATO Advanced Research Workshop on "X-ray Binaries and the Formation of Binary and Millisecond Radio Pulsars" (1991 Santa Barbara, Calif.). X-ray binaries and recycled pulsars. Kluwer Academic Publishers, 1992.

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Heuvel, E. P. J., and S. A. Rappaport, eds. X-Ray Binaries and Recycled Pulsars. Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2704-2.

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Emadzadeh, Amir Abbas, and Jason Lee Speyer. Navigation in Space by X-ray Pulsars. Springer New York, 2011. http://dx.doi.org/10.1007/978-1-4419-8017-5.

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Lee, Speyer Jason, ed. Navigation in Space by X-ray Pulsars. Springer Verlag, 2011.

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Thorsett, Stephen Erik. [X-ray emission from two nearby millisecond pulsars: Final technical report]. California Institute of Technology, 1994.

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Thorsett, Stephen Erik. [X-ray emission from two nearby millisecond pulsars: Final technical report]. California Institute of Technology, 1994.

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Thorsett, Stephen Erik. [X-ray emission from two nearby millisecond pulsars: Final technical report]. California Institute of Technology, 1994.

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M, Cordes James, Yadigaroglu I. -A, and United States. National Aeronautics and Space Administration., eds. X-ray emission from the Guitar Nebula. National Aeronautics and Space Administration, 1997.

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M, Cordes James, Yadigaroglu I. -A, and United States. National Aeronautics and Space Administration., eds. X-ray emission from the Guitar Nebula. National Aeronautics and Space Administration, 1997.

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United States. National Aeronautics and Space Administration, ed. [Analysis and interpretation of X-ray pulsars]: [final technical report]. National Aeronautics and Space Administration, 1987.

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Book chapters on the topic "X-­ray pulsars"

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Walter, Roland, and Carlo Ferrigno. "X-Ray Pulsars." In Handbook of Supernovae. Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-20794-0_74-1.

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Walter, Roland, and Carlo Ferrigno. "X-Ray Pulsars." In Handbook of Supernovae. Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-21846-5_74.

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Feroci, Marco, and Paolo Soffitta. "X-ray Polarimeters." In High-Energy Emission from Pulsars and their Systems. Springer Berlin Heidelberg, 2010. http://dx.doi.org/10.1007/978-3-642-17251-9_48.

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Mereghetti, S. "The Anomalous X-Ray Pulsars." In The Neutron Star—Black Hole Connection. Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-010-0548-7_27.

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Patruno, Alessandro, and Anna L. Watts. "Accreting Millisecond X-ray Pulsars." In Timing Neutron Stars: Pulsations, Oscillations and Explosions. Springer Berlin Heidelberg, 2020. http://dx.doi.org/10.1007/978-3-662-62110-3_4.

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Kulkarni, S. R., J. Navarro, G. Vasisht, Y. Tanaka, and F. Nagase. "Millisecond Pulsars and Quiescent LMXBS." In X-Ray Binaries and Recycled Pulsars. Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2704-2_11.

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Fruchter, A. S., and W. M. Goss. "Continuum Observations of Recycled Pulsars." In X-Ray Binaries and Recycled Pulsars. Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2704-2_12.

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Lyne, A. G. "Millisecond Pulsars in Globular Clusters." In X-Ray Binaries and Recycled Pulsars. Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2704-2_8.

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Taylor, J. H. "Recent Observations of Recycled Pulsars." In X-Ray Binaries and Recycled Pulsars. Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2704-2_9.

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Becker, Werner. "X-Ray Emission from Pulsars and Neutron Stars." In Neutron Stars and Pulsars. Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-540-76965-1_6.

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Conference papers on the topic "X-­ray pulsars"

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Dib, Rim, Victoria M. Kaspi, Fotis P. Gavriil, et al. "Glitches in Anomalous X-ray Pulsars." In 40 YEARS OF PULSARS: Millisecond Pulsars, Magnetars and More. AIP, 2008. http://dx.doi.org/10.1063/1.2900151.

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Israel, G. L., F. Bernardini, M. Burgay, et al. "Transient Phenomena in Anomalous X-ray Pulsars." In 40 YEARS OF PULSARS: Millisecond Pulsars, Magnetars and More. AIP, 2008. http://dx.doi.org/10.1063/1.2900152.

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Tam, Cindy R., Fotis P. Gavriil, Rim Dib, et al. "The Variable X-ray and Near-IR Behavior of the Particularly Anomalous X-ray Pulsar 1E 1048.1–5937." In 40 YEARS OF PULSARS: Millisecond Pulsars, Magnetars and More. AIP, 2008. http://dx.doi.org/10.1063/1.2900160.

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Özel, Feryal, Tolga Güver, Ersin Göğüş, et al. "The Magnetic Fields of Anomalous X-ray Pulsars." In 40 YEARS OF PULSARS: Millisecond Pulsars, Magnetars and More. AIP, 2008. http://dx.doi.org/10.1063/1.2900155.

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Rea, N., S. Zane, R. Turolla, et al. "New results on magnetars' X-ray spectral modeling." In 40 YEARS OF PULSARS: Millisecond Pulsars, Magnetars and More. AIP, 2008. http://dx.doi.org/10.1063/1.2900167.

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Bogdanov, Slavko, Jonathan E. Grindlay, C. Bassa, Z. Wang, A. Cumming, and V. M. Kaspi. "An X-ray View of Radio Millisecond Pulsars." In 40 YEARS OF PULSARS: Millisecond Pulsars, Magnetars and More. AIP, 2008. http://dx.doi.org/10.1063/1.2900321.

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Ray, Paul S., Michael T. Wolff, Paul Demorest, et al. "X-ray and Radio Timing of PSR B1821–24." In 40 YEARS OF PULSARS: Millisecond Pulsars, Magnetars and More. AIP, 2008. http://dx.doi.org/10.1063/1.2900134.

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Archibald, Anne M., Rim Dib, Margaret A. Livingstone, et al. "Red Noise in Anomalous X-ray Pulsar Timing Residuals." In 40 YEARS OF PULSARS: Millisecond Pulsars, Magnetars and More. AIP, 2008. http://dx.doi.org/10.1063/1.2900158.

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Lommen, A., J. Donovan, C. Gwinn, et al. "Observed X-ray∕Radio Correlation in the Vela Pulsar." In 40 YEARS OF PULSARS: Millisecond Pulsars, Magnetars and More. AIP, 2008. http://dx.doi.org/10.1063/1.2900322.

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Mereghetti, S. "The anomalous x-ray pulsars." In X-RAY ASTRONOMY: Stellar Endpoints,AGN, and the Diffuse X-ray Background. AIP, 2001. http://dx.doi.org/10.1063/1.1434635.

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Reports on the topic "X-­ray pulsars"

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Grove, J. E., J. D. Kurfess, B. F. Phlips, M. S. Strickman, and M. P. Ulmer. OSSE Observations of X-Ray Pulsars. Defense Technical Information Center, 1995. http://dx.doi.org/10.21236/ada464467.

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West, Gavin. Shaping X-Ray Pulses at LCLS - Oral Presentation. Office of Scientific and Technical Information (OSTI), 2015. http://dx.doi.org/10.2172/1213173.

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Zholents, A. Electron beam-based sources of ultrashort x-ray pulses. Office of Scientific and Technical Information (OSTI), 2010. http://dx.doi.org/10.2172/990520.

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Huang, Z. Femtosecond X-ray Pulses From a frequency chirped SASE FEL. Office of Scientific and Technical Information (OSTI), 2003. http://dx.doi.org/10.2172/826693.

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Chin, A. H., R. W. Schoenlein, and T. E. Glover. Ultrashort hard x-ray pulses generated by 90 degrees Thomson scattering. Office of Scientific and Technical Information (OSTI), 1997. http://dx.doi.org/10.2172/603713.

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Emma, P. ATTOSECOND X-RAY PULSES IN THE LCLS USING THE SLOTTED FOIL METHOD. Office of Scientific and Technical Information (OSTI), 2004. http://dx.doi.org/10.2172/833050.

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Huang, Zhirong, and Ronald D. Ruth. Fully Coherent X-ray Pulses from a Regenerative Amplifier Free Electron Laser. Office of Scientific and Technical Information (OSTI), 2006. http://dx.doi.org/10.2172/876447.

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Miao, J. Taking X-Ray Diffraction to the Limit: Macromolecular Structures from Femtosecond X-Ray Pulses and Diffraction Microscopy of Cells with Synchrotron Radiation. Office of Scientific and Technical Information (OSTI), 2004. http://dx.doi.org/10.2172/826961.

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Emma, P. Femtosecond and Subfemtosecond X-Ray Pulses from a SASE Based Free-Electron Laser. Office of Scientific and Technical Information (OSTI), 2004. http://dx.doi.org/10.2172/826765.

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Zholents, Alexander. Feasibility analysis for attosecond X-ray pulses at FERMI@ELETTRA free electron laser. Office of Scientific and Technical Information (OSTI), 2004. http://dx.doi.org/10.2172/842992.

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You might also be interested in the extended bibliographies on the topic 'X-­ray pulsars' for particular source types:
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