Multiband emission from pulsar wind nebulae: a possible injection spectrum

作者：Fang J^*; Zhang L

来源：Astronomy & Astrophysics, 2010, 515: A20.

DOI：10.1051/0004-6361/200913615

• gamma rays: ISM
• ISM: individual objects: G0.9+0.1
• ISM: individual objects: MSH 15-52
• ISM: individual objects: G338.3-0.0
• acceleration of praticles
• radiation mechanisms: non-thermal

Aims. Recent research shows that particles with a spectrum of a relativistic Maxwellian plus a high-energy tail can be accelerated by relativistic collisionless shocks. We investigate the possibility of the high-energy particles with this new spectrum injected into pulsar wind nebulae (PWNe) from the terminate shock based on the study of multiwavelength emission from PWNe.
Methods. The dynamics of a supernova remnant (SNR) and multiband nonthermal emission from the PWN inside the remnant are investigated using a dynamical model with electrons/positrons injected with the new spectrum. In this model, the dynamical and radiative evolution of a pulsar wind nebula in a nonradiative supernova remnant can be described self-consistently.
Results. This model is applied to the three composite SNRs, G0.9+0.1, MSH 15-52, G338.3-0.0, and the multiband observed emission from the three PWNe is reproduced.
Conclusions. Our studies on the three remnants provide evidence of a new spectrum of the particles, which are accelerated by the terminate shock and injected into a PWN.

• 出版日期2010-6
• 单位云南大学