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| 1 | 2004IJMPA..19.2385Z |
| 265.000 | 00/2004 | A E L X R C U |
| Zhang, Bing; Mészáros, Peter |
| Gamma-Ray Bursts: progress, problems & prospects |
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| 2 | 2006ApJ...642..354Z |
| 239.000 | 05/2006 | A E F L X R C S N U |
| Zhang, Bing; Fan, Y. Z.; Dyks, Jaroslaw; Kobayashi, Shiho; Mészáros, Peter; Burrows, David N.; Nousek, John A.; Gehrels, Neil |
| Physical Processes Shaping Gamma-Ray Burst X-Ray Afterglow Light Curves: Theoretical Implications from the Swift X-Ray Telescope Observations |
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| 3 | 2002ApJ...571..876Z |
| 129.000 | 06/2002 | A E F L X R C U H |
| Zhang, Bing; Mészáros, Peter |
| Gamma-Ray Burst Beaming: A Universal Configuration with a Standard Energy Reservoir? |
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| 4 | 2000ApJ...532.1150Z |
| 100.000 | 04/2000 | A E F L X D R C S U H |
| Zhang, Bing; Harding, Alice K. |
| Full Polar Cap Cascade Scenario: Gamma-Ray and X-Ray Luminosities from Spin-powered Pulsars |
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| 5 | 2003ApJ...595..950Z |
| 90.000 | 10/2003 | A E F L X R C S N U H |
| Zhang, Bing; Kobayashi, Shiho; Mészáros, Peter |
| Gamma-Ray Burst Early Optical Afterglows: Implications for the Initial Lorentz Factor and the Central Engine |
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| 6 | 2002ApJ...581.1236Z |
| 88.000 | 12/2002 | A E F L X R C S U H |
| Zhang, Bing; Mészáros, Peter |
| An Analysis of Gamma-Ray Burst Spectral Break Models |
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| 7 | 2004ApJ...601L.119Z |
| 72.000 | 02/2004 | A E F L X R C S U H |
| Zhang, Bing; Dai, Xinyu; Lloyd-Ronning, Nicole M.; Mészáros, Peter |
| Quasi-universal Gaussian Jets: A Unified Picture for Gamma-Ray Bursts and X-Ray Flashes |
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| 8 | 2001ApJ...552L..35Z |
| 65.000 | 05/2001 | A E F L X R C S U H |
| Zhang, Bing; Mészáros, Peter |
| Gamma-Ray Burst Afterglow with Continuous Energy Injection: Signature of a Highly Magnetized Millisecond Pulsar |
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| 9 | 2001ApJ...559..110Z |
| 64.000 | 09/2001 | A E F L X R C S N U H |
| Zhang, Bing; Mészáros, Peter |
| High-Energy Spectral Components in Gamma-Ray Burst Afterglows |
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| 10 | 2002ApJ...566..712Z |
| 57.000 | 02/2002 | A E F L X R C S U H |
| Zhang, Bing; Mészáros, Peter |
| Gamma-Ray Bursts with Continuous Energy Injection and Their Afterglow Signature |
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| 11 | 2007ChJAA...7....1Z |
| 52.000 | 02/2007 | A E F G X R C U |
| Zhang, Bing |
| Gamma-Ray Bursts in the Swift Era |
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| 12 | 2005ApJ...628..315Z |
| 52.000 | 07/2005 | A E F L X R C S N U |
| Zhang, Bing; Kobayashi, Shiho |
| Gamma-Ray Burst Early Afterglows: Reverse Shock Emission from an Arbitrarily Magnetized Ejecta |
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| 13 | 2000ApJ...531L.135Z |
| 45.000 | 03/2000 | A E F L X R C S U H |
| Zhang, Bing; Harding, Alice K.; Muslimov, Alexander G. |
| Radio Pulsar Death Line Revisited: Is PSR J2144-3933 Anomalous? |
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| 14 | 2000ApJ...535L..51Z |
| 44.000 | 05/2000 | A E F L X R C S U H |
| Zhang, Bing; Harding, Alice K. |
| High Magnetic Field Pulsars and Magnetars: A Unified Picture |
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| 15 | 2007ApJ...655..989Z |
| 36.000 | 02/2007 | A E F L X R C S N U |
| Zhang, Bing; Liang, Enwei; Page, Kim L.; Grupe, Dirk; Zhang, Bin-Bin; Barthelmy, Scott D.; Burrows, David N.; Campana, Sergio; Chincarini, Guido; Gehrels, Neil; and 10 coauthors |
| GRB Radiative Efficiencies Derived from the Swift Data: GRBs versus XRFs, Long versus Short |
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| 16 | 1997ApJ...478..313Z |
| 32.000 | 03/1997 | A E F L R C S U |
| Zhang, B.; Qiao, G. J.; Lin, W. P.; Han, J. L. |
| Three Modes of Pulsar Inner Gap |
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| 17 | 2007ApJ...655L..25Z |
| 29.000 | 01/2007 | A E F L X R C S N U |
| Zhang, Bing; Zhang, Bin-Bin; Liang, En-Wei; Gehrels, Neil; Burrows, David N.; Mészáros, Peter |
| Making a Short Gamma-Ray Burst from a Long One: Implications for the Nature of GRB 060614 |
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| 18 | 2000ApJ...545L.127Z |
| 26.000 | 12/2000 | A E F L X R C S U H |
| Zhang, Bing; Xu, R. X.; Qiao, G. J. |
| Nature and Nurture: a Model for Soft Gamma-Ray Repeaters |
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| 19 | 1996A&A...310..135Z |
| 24.000 | 06/1996 | A F G R C S U |
| Zhang, B.; Qiao, G. J. |
| A study on pulsar inner-gap sparking comparing inverse Compton scattering and curvature radiation processes. |
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| 20 | 1997ApJ...491..891Z |
| 20.000 | 12/1997 | A E F L R C S U |
| Zhang, B.; Qiao, G. J.; Han, J. L. |
| Inverse Compton Scattering: Gap Parameters, Energy Loss of the Particles, and Possible Implications for Pulsar Radio Emission |
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| 21 | 2005ApJ...624L.109Z |
| 14.000 | 05/2005 | A E F L X R C S U |
| Zhang, Bing; Sanwal, Divas; Pavlov, George G. |
| An XMM-Newton Observation of the Drifting Pulsar B0943+10 |
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| 22 | 2001ApJ...562L..59Z |
| 13.000 | 11/2001 | A E F L X R C S U H |
| Zhang, Bing |
| On the Radio Quiescence of Anomalous X-Ray Pulsars and Soft Gamma-Ray Repeaters |
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| 23 | 2006Natur.444.1010Z |
| 12.000 | 12/2006 | A E L X R C U |
| Zhang, Bing |
| Astrophysics: A burst of new ideas |
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| 24 | 2004ApJ...614L..53Z |
| 12.000 | 10/2004 | A E F L X R C S U H |
| Zhang, Bing; Loeb, Abraham |
| A Model for the Flaring Radio Emission in the Double Pulsar System J0737-3039 |
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| 25 | 1998A&A...338...62Z |
| 12.000 | 10/1998 | A E F G X R C S U |
| Zhang, Bing; Qiao, G. J. |
| Two-photon annihilation in the pair formation cascades in pulsar polar caps |
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| 26 | 2007AdSpR..40.1186Z |
| 11.000 | 00/2007 | A E F L X R C U |
| Zhang, Bing |
| Gamma-ray burst afterglows |
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| 27 | 2003ApJ...595..346Z |
| 11.000 | 09/2003 | A E F L X R C S U H |
| Zhang, Bing; Dai, Z. G.; Mészáros, P.; Waxman, E.; Harding, A. K. |
| High-Energy Neutrinos from Magnetars |
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| 28 | 2007MNRAS.374.1103Z |
| 10.000 | 01/2007 | A E F L X R C S U |
| Zhang, Bing; Gil, Janusz; Dyks, Jaroslaw |
| On the origins of part-time radio pulsars |
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| 29 | 2005ApJ...631L.143Z |
| 9.000 | 10/2005 | A E F L X R C S U |
| Zhang, Bing; Gil, Janusz |
| GCRT J1745-3009 as a Transient White Dwarf Pulsar |
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| 30 | 2003ApJ...596L..95Z |
| 9.000 | 10/2003 | A E F L X R C U H |
| Zhang, Bing; Sigurdsson, Steinn |
| Electromagnetic Signals from Planetary Collisions |
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| 31 | 2003AcASn..44S.215Z |
| 4.000 | 02/2003 | A F L X R C U H |
| Zhang, Bing |
| Radio Pulsar Death |
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| 32 | 1999ApJ...514L.111Z |
| 2.000 | 04/1999 | A E F L X R C U |
| Zhang, Bing; Hong, B. H.; Qiao, G. J. |
| Is Coherence Essential to Account for Pulsar Radio Emission? |
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| 33 | 2006ChJAS...6b..90Z |
| 0.000 | 12/2006 | A F G U |
| Zhang, Bing |
| Possible New Clues towards Understanding Pulsar Radio Emission |
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