Is there room for highly magnetized pulsar wind nebulae among those non-detected at TeV?
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Title
Is there room for highly magnetized pulsar wind nebulae among those non-detected at TeV?
Authors
Keywords
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Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 443, Issue 1, Pages 138-145
Publisher
Oxford University Press (OUP)
Online
2014-07-10
DOI
10.1093/mnras/stu1125
References
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Related references
Note: Only part of the references are listed.- Time-dependent modeling of TeV-detected, young pulsar wind nebulae
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- (2013) S. J. Tanaka et al. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
- The effects of magnetic field, age and intrinsic luminosity on Crab-like pulsar wind nebulae
- (2013) D. F. Torres et al. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
- The near-infrared detection of PSR B0540–69 and its nebula
- (2012) R. P. Mignani et al. ASTRONOMY & ASTROPHYSICS
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- AN ENERGY-CONSERVING, PARTICLE-DOMINATED, TIME-DEPENDENT MODEL OF 3C 58 AND ITS OBSERVABILITY AT HIGH ENERGIES
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- Time-dependent modelling of pulsar wind nebulae: study on the impact of the diffusion-loss approximations
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- (2011) Z. Arzoumanian et al. ASTROPHYSICAL JOURNAL
- STUDY OF FOUR YOUNG TeV PULSAR WIND NEBULAE WITH A SPECTRAL EVOLUTION MODEL
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- DISCOVERY OF A HIGHLY ENERGETIC PULSAR ASSOCIATED WITH IGR J14003–6326 IN THE YOUNG UNCATALOGED GALACTIC SUPERNOVA REMNANT G310.6–1.6
- (2010) M. Renaud et al. ASTROPHYSICAL JOURNAL
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- (2008) Z. Arzoumanian et al. ASTROPHYSICAL JOURNAL
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