Xu, Ren-Xin - Department of Astronomy, Peking University

• arXiv:1101.2289v1[astro-ph.HE]12Jan2011 AXPs and SGRs in the outer gap model: confronting Fermi
• What if pulsars are born as strange stars? R.X. Xu a,b
• arXiv:astro-ph/9912303v24Apr2000 Vacuum discharge as a possible source of gamma-ray bursts
• ############# 1 Pulsars#Neutron Stars or Strange Stars#
• Vol.44 Suppl. ACTA ASTRONOMICA SINICA Feb., 2003 Strange Quark Stars
• Research in Astron. Astrophys. 2010 Vol. 10 No. 6, 553568 http://www.raa-journal.org http://www.iop.org/journals/raa
• Mon. Not. R. Astron. Soc. 402, 27152719 (2010) doi:10.1111/j.1365-2966.2009.16091.x Strange stars with different quark mass scalings
• PA2. Neutron stars "PA2. NSs" http://vega.bac.pku.edu.cn/rxxu R. X. Xu
• Mon. Not. R. Astron. Soc. 384, 10341038 (2008) doi:10.1111/j.1365-2966.2007.12575.x Pulsar slow glitches in a solid quark star model
• To probe into pulsar's interior through gravitational waves Department of Astronomy, School of Physics, Peking University, Beijing 100871, China
• 1. Important Information...................................................................II 1.1 Meeting room for CSQCDII.........................................................................II
• Mon. Not. R. Astron. Soc. 356, 359370 (2005) doi:10.1111/j.1365-2966.2004.08437.x 1E 1207.4-5209: a low-mass bare strange star?
• Low-mass bare strange stars School of Physics, Peking University, Beijing 100871, China
• . Research Paper . SCIENCE CHINA
• Author's personal copy AXPs/SGRs: Magnetars or quark-stars?
• SWIFT J1749.42807: A neutron or quark star? This article has been downloaded from IOPscience. Please scroll down to see the full text article.
• Chin. J. Astron. Astrophys. Vol. 3 (2003), No. 1, 3337 ( http://www.chjaa.org or http://chjaa.bao.ac.cn )
• Mon. Not. R. Astron. Soc. 412, 26782684 (2011) doi:10.1111/j.1365-2966.2010.18104.x Hurst parameter analysis of radio pulsar timing residuals
• A&A 407, L25L28 (2003) DOI: 10.1051/0004-6361:20031055
• Mon. Not. R. Astron. Soc. 366, 945952 (2006) doi:10.1111/j.1365-2966.2005.09743.x Observational constraints on the radio and -ray emission regions
• CHIN.PHYS.LETT. Vol. 20, No. 6 (2003) 806 Ultra High Energy Cosmic Rays: Strangelets?
• Astron. Astrophys. 323, 395--398 (1997) ASTRONOMY ASTROPHYSICS
• Mon. Not. R. Astron. Soc. 373, L85L89 (2006) doi:10.1111/j.1745-3933.2006.00248.x The superflares of soft -ray repeaters: giant quakes in solid quark stars?
• A note on the discovery of a 2M pulsar This article has been downloaded from IOPscience. Please scroll down to see the full text article.
• Mon. Not. R. Astron. Soc. 381, L1L5 (2007) doi:10.1111/j.1745-3933.2007.00337.x PSR B1828-11: a precession pulsar torqued by a quark planet?
• Mon. Not. R. Astron. Soc. 405, 27542758 (2010) doi:10.1111/j.1365-2966.2010.16660.x Microlensing pulsars
• Chin. J. Astron. Astrophys. Vol. 6 (2006), Suppl.2, 287290 (http://www.chjaa.org)
• CPC(HEP & NP), 2010, 34(9): 13311334 Chinese Physics C Vol. 34, No. 9, Sep., 2010 Quark-clustering in cold quark matter*
• High Energy Processes and Phenomena in Astrophysics IAU Symposium, Vol. 214, 2003
• Author's personal copy What can the braking indices tell us about the nature of pulsars?
• A note on solid pulsars School of Physics, Peking University, Beijing 100871, China
• The Astrophysical Journal, 570:L65L68, 2002 May 10 2002. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• The Astrophysical Journal, 596:L75L78, 2003 October 10 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• The Astrophysical Journal Letters, 725:L196L199, 2010 December 20 doi:10.1088/2041-8205/725/2/L196 C 2010. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
• \Delta 21 \Delta 2 I \Theta p \Theta @ \Theta ---\Theta ( Vol.21, \Delta No.2 \Delta \Delta \Delta 2003 6 PROGRESS IN ASTRONOMY Jun., 2003 \Delta
• Mon. Not. R. Astron. Soc. 401, 14651474 (2010) doi:10.1111/j.1365-2966.2009.15760.x Towards the properties of long gamma-ray burst progenitors
• CPC(HEP & NP), 2011, 35(7): 616621 Chinese Physics C Vol. 35, No. 7, Jul., 2011 A new parametric equation of state and quark stars*
• The Astrophysical Journal, 703:507516, 2009 September 20 doi:10.1088/0004-637X/703/1/507 C 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
• Quakes in solid quark stars A.Z. Zhou a
• ASTROPHYSICS Thesaurus of key words used in the annual subject indexes
• Physics and Classification
• A Series Journal of the Chinese Physical Society Distributed by IOP Publishing
• Chin. J. Astron. Astrophys. Vol. 6 (2006), Suppl.2, 279286 (http://www.chjaa.org)
• The Astrophysical Journal, 596:L59L62, 2003 October 10 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• Chin. J. Astron. Astrophys. Vol. 5 (2005), Suppl., 353358 (http://www.chjaa.org)
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• arXiv e-print (arXiv:1103.0389) L. Landau 1908 1962
• The Astrophysical Journal, 522:L109L112, 1999 September 10 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• THE ASTROPHYSICAL JOURNAL, 535:354364, 2000 May 20 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
• V O ~ . 43 NO. 4 SCIENCE IN CHINA (Series A) ~ p r i l2000 Are there real orthogonal polarization modes in pulsar radio
• The Astrophysical Journal, 545:L127L130, 2000 December 20 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• A&A 371, 963972 (2001) DOI: 10.1051/0004-6361:20010450
• The Astrophysical Journal, 561:L85L88, 2001 November 1 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• Chin. J. Astron. Astrophys. Vol. 2 (2002), No. 6, 533{538 (http://www.chjaa.org or http://chjaa.bao.ac.cn )
• A&A 387, 710713 (2002) DOI: 10.1051/0004-6361:20020395
• POSSIBLE EVIDENCE FOR PULSED X-RAY EMISSION FROM THE OUTER GAP IN PSR B1937+21 H. G. Wang, R. X. Xu, and G. J. Qiao
• ( ) , 39 , 3 ,2003 ~OE 5 Acta Scientiarum Naturalium
• A&A 409, 641645 (2003) DOI: 10.1051/0004-6361:20031188
• The Astrophysical Journal, 606:L49L52, 2004 May 1 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• The Astrophysical Journal, 616:L127L130, 2004 December 1 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• Mon. Not. R. Astron. Soc. 365, L16L20 (2006) doi:10.1111/j.1745-3933.2005.00117.x GCRT J1745-3009: a precessing radio pulsar?
• Chin. J. Astron. Astrophys. Vol. 6 (2006), No. 5, 572578 (http://www.chjaa.org)
• IOP PUBLISHING JOURNAL OF PHYSICS G: NUCLEAR AND PARTICLE PHYSICS J. Phys. G: Nucl. Part. Phys. 34 (2007) 597605 doi:10.1088/0954-3899/34/3/017
• A&A 472, 13 (2007) DOI: 10.1051/0004-6361:20077200
• This article appeared in a journal published by Elsevier. The attached copy is furnished to the author for internal non-commercial research
• Science in China Series G: Physics, Mechanics & Astronomy 2009 SCIENCE IN CHINA PRESS
• Mon. Not. R. Astron. Soc. 398, L31L35 (2009) doi:10.1111/j.1745-3933.2009.00701.x Lennard-Jones quark matter and massive quark stars
• Mon. Not. R. Astron. Soc. 399, 15871596 (2009) doi:10.1111/j.1365-2966.2009.15373.x The formation of submillisecond pulsars and the possibility of detection
• Mon. Not. R. Astron. Soc. 414, 489494 (2011) doi:10.1111/j.1365-2966.2011.18409.x Magnetospheric activity of bare strange quark stars
• arXiv:1104.0080v1[astro-ph.HE]1Apr2011 Plateaus of gamma-ray bursts and supernovae: A unified
• arXiv:1104.5287v1[astro-ph.HE]28Apr2011 Preprint typeset using LATEX style emulateapj v. 01/26/10
• LOW-MASS QUARK STARS School of Physics, Peking University, Beijing 100871, China; E-mail: r.x.xu@pku.edu.cn
• IOP PUBLISHING JOURNAL OF PHYSICS G: NUCLEAR AND PARTICLE PHYSICS J. Phys. G: Nucl. Part. Phys. 36 (2009) 064010 (9pp) doi:10.1088/0954-3899/36/6/064010
• Neutron Star Matter Including Delta Isobars Guang-Zhou Liu1,2
• Differential-Rotation Law of Slowly Rotating Star Jianyong Shen
• Compact stars in the QCD phase diagram II (CSQCD II) May 20-24, 2009, KIAA at Peking University, Beijing -P. R. China
• 23 2 Vol.23, No.2 2005 6 PROGRESS IN ASTRONOMY Jun., 2005
• Compact stars in the QCD phase diagram II Beijing, China, May 20-24th, 2009
• This article appeared in a journal published by Elsevier. The attached copy is furnished to the author for internal non-commercial research
• Mon. Not. R. Astron. Soc. 410, 14411446 (2011) doi:10.1111/j.1365-2966.2010.17512.x Can eccentric binary millisecond pulsars form by accretion-induced
• JCAP05(2010)028 ournal of Cosmology and Astroparticle Physics
• The Astrophysical Journal, 649: L95L98, 2006 October 1 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• Chin. J. Astron. Astrophys. Vol. 1, No. 1, (2001) 001--100 Chinese Journal of Astronomy and
• Compact stars in the QCD phase diagram II (CSQCD II) May 20-24, 2009, KIAA at Peking University, Beijing -P. R. China
• Chin. J. Astron. Astrophys. Vol. 6 (2006), No. 2, 217226 (http://www.chjaa.org)
• The Astrophysical Journal, 668: L55L58, 2007 October 10 2007. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• Circular polarization in pulsar integrated profiles J. L. Han,1
• arXiv:1109.0665v2[physics.gen-ph]7Sep2011 September 8, 2011 0:57 WSPC/INSTRUCTION FILE ms
• arXiv:1107.0834v1[astro-ph.SR]5Jul2011 H-cluster stars
• arXiv:1107.0830v1[astro-ph.HE]5Jul2011 Research in Astron. Astrophys. 2009 Vol. 9 No. XX, 000000
• arXiv:1110.1226v1[astro-ph.HE]6Oct2011 Absorption features caused by oscillations of electrons on the surface of a quark star
• arXiv:1110.1975v2[astro-ph.HE]14Nov2011 November 15, 2011 1:17 WSPC/INSTRUCTION FILE ms