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Journal articles on the topic 'EXO 0748-676'

Author: Grafiati
Published: 9 March 2023

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1

RODRIGUES, H., S. B. DUARTE, and J. C. T. OLIVEIRA. "EXO 0748-676 AS A QUARK STAR." International Journal of Modern Physics D 19, no. 08n10 (August 2010): 1447–54. http://dx.doi.org/10.1142/s0218271810017500.

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This work shows results for the EXO 0748-676 neutron star structure obtained with the use of a phenomenological quark matter description by taking into account a quark interaction, and observing the asymptotic freedom and the confinement characteristics of the fundamental theory. An appropriated choice of model parameters permit to reach the stability of compact dense stellar objects compatible with the observational data to the neutron star EXO 0748-676. It is assumed a color-flavor locked (CFL) superconducting phase to the ground state of the quark–gluon plasma formed in the object interior. We also discuss the surface properties of these objects, introducing a crust composed by a lattice of neutron-rich nucleus close to the neutron drip line, imbedded in an electron gas.
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2

Hynes, R. I., C. A. Haswell, E. L. Robinson, K. Horne, K. O'Brien, P. A. Charles, A. R. King, and D. J. Rolfe. "Disentangling X-Ray Reprocessing Sites in EXO 0748-676." International Astronomical Union Colloquium 194 (2004): 12–13. http://dx.doi.org/10.1017/s0252921100151723.

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AbstractWe present first results from a coordinated multiwavelength study of the neutron star low-mass X-ray binary EXO 0748 676. Fast UV, X-ray, and optical data were obtained including both spectral and timing information. We discuss how this study allows us to probe the temperature distribution within the binary and hence the geometry and efficiency of X-ray irradiation.
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3

Jain, Chetana, and Biswajit Paul. "Search for pulsations in the LMXB EXO 0748–676." Research in Astronomy and Astrophysics 11, no. 5 (April 20, 2011): 577–82. http://dx.doi.org/10.1088/1674-4527/11/5/007.

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4

Pearson, K. J., R. I. Hynes, D. Steeghs, P. G. Jonker, C. A. Haswell, A. R. King, K. O’Brien, G. Nelemans, and M. Mendez. "Multiwavelength Observations of EXO 0748−676. II. Emission‐Line Behavior." Astrophysical Journal 648, no. 2 (September 10, 2006): 1169–80. http://dx.doi.org/10.1086/506191.

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5

Bassa, C. G., P. G. Jonker, D. Steeghs, and M. A. P. Torres. "Optical spectroscopy of the quiescent counterpart to EXO���0748���676." Monthly Notices of the Royal Astronomical Society 399, no. 4 (November 11, 2009): 2055–62. http://dx.doi.org/10.1111/j.1365-2966.2009.15395.x.

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6

Wade, R. A., H. Quintana, K. Horne, and T. R. Marsh. "Optical studies of the X-ray transient EXO 0748-676." Publications of the Astronomical Society of the Pacific 97 (November 1985): 1092. http://dx.doi.org/10.1086/131668.

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7

Boirin, L., L. Keek, M. Méndez, A. Cumming, J. J. M. In 't Zand, J. Cottam, F. Paerels, and W. H. G. Lewin. "Discovery of X-ray burst triplets in EXO 0748-676." Astronomy & Astrophysics 465, no. 2 (January 22, 2007): 559–73. http://dx.doi.org/10.1051/0004-6361:20066204.

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8

Xu, Ren-Xin. "What Can the Redshift Observed in EXO 0748–676 Tell Us?" Chinese Journal of Astronomy and Astrophysics 3, no. 1 (February 2003): 33–37. http://dx.doi.org/10.1088/1009-9271/3/1/33.

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9

Degenaar, N., Z. Medin, A. Cumming, R. Wijnands, M. T. Wolff, E. M. Cackett, J. M. Miller, P. G. Jonker, J. Homan, and E. F. Brown. "PROBING THE CRUST OF THE NEUTRON STAR IN EXO 0748-676." Astrophysical Journal 791, no. 1 (July 25, 2014): 47. http://dx.doi.org/10.1088/0004-637x/791/1/47.

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10

Muñoz-Darias, T., J. Casares, K. O'Brien, D. Steeghs, I. G. Martínez-Pais, R. Cornelisse, and P. A. Charles. "Dynamical constraints on the neutron star mass in EXO 0748−676." Monthly Notices of the Royal Astronomical Society: Letters 394, no. 1 (March 21, 2009): L136—L140. http://dx.doi.org/10.1111/j.1745-3933.2009.00630.x.

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11

Villarreal, Adam R., and Tod E. Strohmayer. "Discovery of the Neutron Star Spin Frequency in EXO 0748-676." Astrophysical Journal 614, no. 2 (September 16, 2004): L121—L124. http://dx.doi.org/10.1086/425737.

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12

Knight, Amy H., Adam Ingram, Matthew Middleton, and Jeremy Drake. "Eclipse mapping of EXO 0748–676: evidence for a massive neutron star." Monthly Notices of the Royal Astronomical Society 510, no. 4 (December 23, 2021): 4736–56. http://dx.doi.org/10.1093/mnras/stab3722.

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ABSTRACT Determining the maximum possible neutron star (NS) mass places limits on the equation of state (EoS) of ultra-dense matter. The mass of NSs in low-mass X-ray binaries can be determined from the binary mass function, providing independent constraints are placed on both the binary inclination and mass ratio. In eclipsing systems, they relate via the totality duration. EXO 0748–676 is an eclipsing NS low-mass X-ray binary with a binary mass function estimated using stellar emission lines from the irradiated face of the companion. The NS mass is thus known as a function of mass ratio. Here, we model the X-ray eclipses in several energy bands, utilizing archival XMM–Newton data. We find a narrow region of absorbing material surrounding the companion star is required to explain the energy-dependent eclipses. Therefore, we suggest the companion may be experiencing ablation of its outer layers and that the system could transition into a redback millisecond pulsar. Our fit returns a mass ratio of $q=0.222^{+0.07}_{-0.08}$ and an inclination $i = 76.5 \pm ^{1.4}_{1.1}$. Combining these with the previously measured radial velocity of 410 ± 5 km s−1, derived from Doppler mapping analysis of H α emission during quiescence, returns an NS mass of ∼2 M⊙ even if the line originates as far from the NS as physically possible, favouring hard EoS. The inferred mass increases for a more realistic emission point. However, a ∼1.4 M⊙ canonical NS mass is possible when considering radial velocity values derived from other emission lines observed both during outburst and quiescence.
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13

Schmidtke, Paul C., and A. P. Cowley. "The variable light curve of the X-ray transient EXO 0748 - 676." Astronomical Journal 93 (February 1987): 374. http://dx.doi.org/10.1086/114322.

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14

Hynes, Robert I., and Erica D. Jones. "THE QUIESCENT OPTICAL AND INFRARED COUNTERPART TO EXO 0748-676 = UY VOL." Astrophysical Journal 697, no. 1 (April 29, 2009): L14—L17. http://dx.doi.org/10.1088/0004-637x/697/1/l14.

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15

Cottam, J., F. Paerels, M. Mendez, L. Boirin, W. H. G. Lewin, E. Kuulkers, and J. M. Miller. "The Burst Spectra of EXO 0748−676 during a Long 2003XMM‐NewtonObservation." Astrophysical Journal 672, no. 1 (January 2008): 504–9. http://dx.doi.org/10.1086/524186.

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16

Hynes, R. I., Keith Horne, K. O’Brien, C. A. Haswell, E. L. Robinson, A. R. King, P. A. Charles, and K. J. Pearson. "Multiwavelength Observations of EXO 0748–676. I. Reprocessing of X‐Ray Bursts." Astrophysical Journal 648, no. 2 (September 10, 2006): 1156–68. http://dx.doi.org/10.1086/505592.

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17

Mikles, Valerie J., and Robert I. Hynes. "GEMINI MULTI-OBJECT SPECTROGRAPH SPECTROSCOPY OF EXO 0748–676 (=UY Vol) IN OUTBURST." Astrophysical Journal 750, no. 2 (April 24, 2012): 132. http://dx.doi.org/10.1088/0004-637x/750/2/132.

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18

Wolff, Michael T., Kent S. Wood, and Paul S. Ray. "Possible Magnetic Activity in the Low-Mass X-Ray Binary EXO 0748-676." Astrophysical Journal 668, no. 2 (October 2, 2007): L151—L154. http://dx.doi.org/10.1086/522833.

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19

Zhang, Zhongli, Soki Sakurai, Kazuo Makishima, Kazuhiro Nakazawa, Ko Ono, Shin’ya Yamada, and Haiguang Xu. "SUZAKUOBSERVATION OF THE HIGH-INCLINATION BINARY EXO 0748–676 IN THE HARD STATE." Astrophysical Journal 823, no. 2 (May 31, 2016): 131. http://dx.doi.org/10.3847/0004-637x/823/2/131.

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20

Bonnet-Bidaud, J. M., F. Haberl, P. Ferrando, P. J. Bennie, and E. Kendziorra. "The eclipsing bursting X-ray binary EXO 0748-676 revisited by XMM-Newton." Astronomy & Astrophysics 365, no. 1 (January 2001): L282—L287. http://dx.doi.org/10.1051/0004-6361:20000222.

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21

Crampton, D., J. Stauffer, J. B. Hutchings, A. P. Cowley, and P. Ianna. "Optical observations of the X-ray nova EXO 0748-676 near maximum light." Astrophysical Journal 306 (July 1986): 599. http://dx.doi.org/10.1086/164369.

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22

Parikh, A. S., N. Degenaar, J. V. Hernández Santisteban, R. Wijnands, I. Psaradaki, E. Costantini, D. Modiano, and J. M. Miller. "UV and X-ray observations of the neutron star LMXB EXO 0748–676 in its quiescent state." Monthly Notices of the Royal Astronomical Society 501, no. 1 (December 3, 2020): 1453–62. http://dx.doi.org/10.1093/mnras/staa3734.

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ABSTRACT The accretion behaviour in low-mass X-ray binaries (LMXBs) at low luminosities, especially at <1034 erg s−1, is not well known. This is an important regime to study to obtain a complete understanding of the accretion process in LMXBs, and to determine if systems that host neutron stars with accretion-heated crusts can be used probe the physics of dense matter (which requires their quiescent thermal emission to be uncontaminated by residual accretion). Here, we examine ultraviolet (UV) and X-ray data obtained when EXO 0748–676, a crust-cooling source, was in quiescence. Our Hubble Space Telescope spectroscopy observations do not detect the far-UV continuum emission, but do reveal one strong emission line, C iv. The line is relatively broad (≳3500 km s−1), which could indicate that it results from an outflow such as a pulsar wind. By studying several epochs of X-ray and near-UV data obtained with XMM–Newton, we find no clear indication that the emission in the two wavebands is connected. Moreover, the luminosity ratio of LX/LUV ≳ 100 is much higher than that observed from neutron star LMXBs that exhibit low-level accretion in quiescence. Taken together, this suggests that the UV and X-ray emission of EXO 0748–676 may have different origins, and that thermal emission from crust-cooling of the neutron star, rather than ongoing low-level accretion, may be dominating the observed quiescent X-ray flux evolution of this LMXB.
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23

Díaz Trigo, M., L. Boirin, E. Costantini, M. Méndez, and A. Parmar. "XMM-Newtonobservations of the low-mass X-ray binary EXO 0748−676 in quiescence." Astronomy & Astrophysics 528 (March 18, 2011): A150. http://dx.doi.org/10.1051/0004-6361/201016200.

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24

Psaradaki, I., E. Costantini, M. Mehdipour, and M. Díaz Trigo. "Modelling the disc atmosphere of the low mass X-ray binary EXO 0748-676." Astronomy & Astrophysics 620 (December 2018): A129. http://dx.doi.org/10.1051/0004-6361/201834000.

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Low mass X-ray binaries exhibit ionized emission from an extended disc atmosphere that surrounds the accretion disc. However, the atmosphere’s nature and geometry is still unclear. In this work we present a spectral analysis of the extended atmosphere of EXO 0748-676 using high-resolution spectra from archival XMM-Newton observations. We model the spectrum that is obtained during the eclipses. This enables us to model the emission lines that come only from the extended atmosphere of the source, and study its physical structure and properties. The RGS spectrum reveals a series of emission lines consistent with transitions of OVIII, OVII, NeIX and NVII. We perform both Gaussian line fitting and photoionization modelling. Our results suggest that there are two photoionization gas components that are out of pressure equilibrium with respect to each other. One has an ionization parameter of log ξ ∼ 2.5 and a large opening angle, and one has log ξ ∼ 1.3. The second component possibly covers a smaller fraction of the source. From the density diagnostics of the OVII triplet using photoionization modelling, we detect a rather high density plasma of > 1013 cm−3 for the lower ionization component. This latter component also displays an inflow velocity. We propose a scenario where the high ionization component constitutes an extended upper atmosphere of the accretion disc. The lower ionization component may instead be a clumpy gas created from the impact of the accretion stream with the disc.
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25

Corbet, R. H. D., K. Asai, T. Dotani, and F. Nagase. "Is the changing orbital period of EXO 0748-676 evidence for a triple system?" Astrophysical Journal 436 (November 1994): L15. http://dx.doi.org/10.1086/187622.

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26

Özel, F. "Soft equations of state for neutron-star matter ruled out by EXO 0748 - 676." Nature 441, no. 7097 (June 2006): 1115–17. http://dx.doi.org/10.1038/nature04858.

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27

Ratti, E. M., D. T. H. Steeghs, P. G. Jonker, M. A. P. Torres, C. G. Bassa, and F. Verbunt. "Optical spectroscopy of the quiescent counterpart to EXO 0748−676: a black widow scenario?" Monthly Notices of the Royal Astronomical Society 420, no. 1 (November 28, 2011): 75–83. http://dx.doi.org/10.1111/j.1365-2966.2011.19999.x.

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28

Shao, Guo-yun, and Yu-xin Liu. "Recalibration of the parameters of EXO 0748-676 and antikaon condensation in neutron star." Physics Letters B 682, no. 2 (November 2009): 171–76. http://dx.doi.org/10.1016/j.physletb.2009.11.007.

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29

Dotani, Tadayasu, and Kazumi Asai. "Effects of the photo-ionized absorber on the continuum spectra of EXO 0748–676." Advances in Space Research 38, no. 12 (January 2006): 2752–55. http://dx.doi.org/10.1016/j.asr.2006.09.013.

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30

Degenaar, N., R. Wijnands, M. T. Wolff, P. S. Ray, K. S. Wood, J. Homan, W. H. G. Lewin, et al. "ChandraandSwiftobservations of the quasi-persistent neutron star transient EXO 0748−676 back to quiescence." Monthly Notices of the Royal Astronomical Society: Letters 396, no. 1 (June 11, 2009): L26—L30. http://dx.doi.org/10.1111/j.1745-3933.2009.00655.x.

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31

Mancuso, G. C., D. Altamirano, F. García, M. Lyu, M. Méndez, J. A. Combi, M. Díaz-Trigo, and J. J. M. in’t Zand. "Discovery of millihertz quasi-periodic oscillations in the X-ray binary EXO 0748−676." Monthly Notices of the Royal Astronomical Society: Letters 486, no. 1 (May 10, 2019): L74—L79. http://dx.doi.org/10.1093/mnrasl/slz057.

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32

Wolff, Michael T., Peter A. Becker, Paul S. Ray, and Kent S. Wood. "A Strong X‐Ray Burst from the Low‐Mass X‐Ray Binary EXO 0748−676." Astrophysical Journal 632, no. 2 (October 20, 2005): 1099–103. http://dx.doi.org/10.1086/444348.

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33

Thomas, Brian, Robin Corbet, Alan P. Smale, Kazumi Asai, and Tadayasu Dotani. "Discovery of a New Soft X-Ray Excess in the Spectrum of EXO 0748−676." Astrophysical Journal 480, no. 1 (May 1, 1997): L21—L25. http://dx.doi.org/10.1086/310611.

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34

Lin, Jinrong, Feryal Özel, Deepto Chakrabarty, and Dimitrios Psaltis. "THE INCOMPATIBILITY OF RAPID ROTATION WITH NARROW PHOTOSPHERIC X-RAY LINES IN EXO 0748–676." Astrophysical Journal 723, no. 2 (October 18, 2010): 1053–56. http://dx.doi.org/10.1088/0004-637x/723/2/1053.

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35

Thomas, Brian, Robin Corbet, Thomas Augusteijn, Paul Callanan, and Alan P. Smale. "Optical and X-ray observations of the low-mass X-ray binary EXO 0748-676." Astrophysical Journal 408 (May 1993): 651. http://dx.doi.org/10.1086/172624.

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36

Parikh, A. S., R. Wijnands, J. Homan, N. Degenaar, B. Wolvers, L. S. Ootes, and D. Page. "Unexpected late-time temperature increase observed in the two neutron star crust-cooling sources XTE J1701−462 and EXO 0748−676." Astronomy & Astrophysics 638 (June 2020): L2. http://dx.doi.org/10.1051/0004-6361/202038198.

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Transient low-mass X-ray binaries (LMXBs) that host neutron stars (NSs) provide excellent laboratories for probing the dense matter physics present in NS crusts. During accretion outbursts in LMXBs, exothermic reactions may heat the NS crust, disrupting the crust-core equilibrium. When the outburst ceases, the crust cools to restore thermal equilibrium with the core. Monitoring this cooling evolution allows us to probe the dense matter physics in the crust. Properties of the deeper crustal layers can be probed at later times after the end of the outburst. We report on the unexpected late-time temperature evolution (≳2000 days after the end of their outbursts) of two NSs in LMXBs, XTE J1701−462 and EXO 0748−676. Although both these sources exhibited very different outbursts (in terms of duration and the average accretion rate), they exhibit an unusually steep decay of ∼7 eV in the observed effective temperature (occurring in a time span of ∼700 days) around ∼2000 days after the end of their outbursts. Furthermore, they both showed an even more unexpected rise of ∼3 eV in temperature (over a time period of ∼500–2000 days) after this steep decay. This rise was significant at the 2.4σ and 8.5σ level for XTE J1701−462 and EXO 0748−676, respectively. The physical explanation for such behaviour is unknown and cannot be straightforwardly be explained within the cooling hypothesis. In addition, this observed evolution cannot be well explained by low-level accretion either without invoking many assumptions. We investigate the potential pathways in the theoretical heating and cooling models that could reproduce this unusual behaviour, which so far has been observed in two crust-cooling sources. Such a temperature increase has not been observed in the other NS crust-cooling sources at similarly late times, although it cannot be excluded that this might be a result of the inadequate sampling obtained at such late times.
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37

Garcia, Michael R., and Paul J. Callanan. "Two Neutron Star Soft X-Ray Transients in Quiescence: 4U 2129+47 and EXO 0748−676." Astronomical Journal 118, no. 3 (September 1999): 1390–94. http://dx.doi.org/10.1086/301014.

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38

Homan, Jeroen, and Michiel van der Klis. "A 695 Hz Quasi‐periodic Oscillation in the Low‐Mass X‐Ray Binary EXO 0748−676." Astrophysical Journal 539, no. 2 (August 20, 2000): 847–50. http://dx.doi.org/10.1086/309280.

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39

Zhang, Guobao, Mariano Méndez, Peter Jonker, and Beike Hiemstra. "The distance and internal composition of the neutron star in EXO 0748−676 with XMM-Newton." Monthly Notices of the Royal Astronomical Society 414, no. 2 (April 6, 2011): 1077–81. http://dx.doi.org/10.1111/j.1365-2966.2011.18443.x.

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40

Parmar, A. N., A. P. Smale, F. Verbunt, and R. H. D. Corbet. "The orbital ephemeris and eclipse transitions of the low-mass X-ray binary EXO 0748 - 676." Astrophysical Journal 366 (January 1991): 253. http://dx.doi.org/10.1086/169557.

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41

Sidoli, L., A. N. Parmar, and T. Oosterbroek. "The broad-band X-ray spectrum of the dipping low mass X-ray binary EXO 0748–676." Astronomy & Astrophysics 429, no. 1 (December 13, 2004): 291–96. http://dx.doi.org/10.1051/0004-6361:20047023.

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42

Galloway, Duncan K., Jinrong Lin, Deepto Chakrabarty, and Jacob M. Hartman. "DISCOVERY OF A 552 Hz BURST OSCILLATION IN THE LOW-MASS X-RAY BINARY EXO 0748–676." Astrophysical Journal 711, no. 2 (February 23, 2010): L148—L151. http://dx.doi.org/10.1088/2041-8205/711/2/l148.

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43

Degenaar, N., M. T. Wolff, P. S. Ray, K. S. Wood, J. Homan, W. H. G. Lewin, P. G. Jonker, et al. "Further X-ray observations of EXO 0748−676 in quiescence: evidence for a cooling neutron star crust." Monthly Notices of the Royal Astronomical Society 412, no. 3 (March 17, 2011): 1409–18. http://dx.doi.org/10.1111/j.1365-2966.2010.17562.x.

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44

Raman, Gayathri, and Biswajit Paul. "X-ray and optical orbital modulation of EXO 0748-676: A co-variability study using XMM-Newton." New Astronomy 54 (July 2017): 122–39. http://dx.doi.org/10.1016/j.newast.2017.02.001.

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45

Gottwald, Manfred, Frank Haberl, Arvind N. Parmar, and Nick E. White. "The properties of bursts with short recurrence times from the transient X-ray source EXO 0748-676." Astrophysical Journal 323 (December 1987): 575. http://dx.doi.org/10.1086/165854.

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46

Parikh, A. S., N. Degenaar, J. V. Hernández Santisteban, R. Wijnands, I. Psaradaki, E. Costantini, D. Modiano, and J. M. Miller. "Erratum: UV and X-ray observations of the neutron star LMXB EXO 0748−676 in its quiescent state." Monthly Notices of the Royal Astronomical Society 502, no. 2 (February 13, 2021): 2826–27. http://dx.doi.org/10.1093/mnras/stab188.

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47

Cheng, Zheng, Mariano Méndez, María Díaz-Trigo, and Elisa Costantini. "The cooling, mass and radius of the neutron star in EXO 0748−676 in quiescence with XMM–Newton." Monthly Notices of the Royal Astronomical Society 471, no. 3 (June 12, 2017): 2605–15. http://dx.doi.org/10.1093/mnras/stx1452.

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48

Hertz, Paul, Kent S. Wood, and Lynn Cominsky. "Eclipse timings of the low-mass X-ray binary EXO 0748-676: Statistical arguments against orbital period changes." Astrophysical Journal 438 (January 1995): 385. http://dx.doi.org/10.1086/175082.

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49

Kotze, M. M., P. A. Charles, and L. A. Crause. "Discovery of long-term superorbital periodicities in the pseudo-transient LMXBs: IGR J17098−3628 and EXO 0748−676." Monthly Notices of the Royal Astronomical Society 395, no. 3 (May 21, 2009): 1579–84. http://dx.doi.org/10.1111/j.1365-2966.2009.14640.x.

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50

Homan, J., R. Wijnands, and M. van den Berg. "XMM-Newton light curves of the low-mass X-ray binary EXO 0748–676: Dips, eclipses, and bursts." Astronomy & Astrophysics 412, no. 3 (December 2003): 799–812. http://dx.doi.org/10.1051/0004-6361:20031484.

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